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C Y G N U S |
Mythology and history
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The origin of the representation as bird of these stars is Greek. It is
thought that the original figure of the mesopotámica tradition had taken the
name of Urakhga, prototype of the Rukh Arab, more known in the West
like the great "Roc", a fiction personage inspired by the merchants of
Bagdad, the story of Simbad the Sailor, content in Thousands and the One
Nights. |
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Characteristics
Cygnus covers a zone with the very great sky and is included/understood if the graph in a square zone is observed. One is a boreal constellation that crosses the observable parallel +40º during the months of spring, summer and part of the autumn in the North hemisphere and the austral one during the very low winter on the horizon. It limits the north with Cepheus and Draco, the east with Lyra, the south with Vulpecula and Pegasus and the west with Lacerta. In addition it crosses the equator of the Milky Route reason why rich in stars shining, stellar clusters gorgeous variable and cloudy stars, in addition to agglomerations of novae and supernovae is one. It is characterized sometimes by its cross form denominating itself, cross of the north, destancando its star more shining Deneb, white and supergiant, 60,000 times greater than our Sun.
Vista from the Earth the zone of Cygnus corresponds to an external spiral arm, in opposite direction al nucleus of the Milky Route, that is to about 4,000 years light of us. It is necessary to emphasize that the nucleus of the Milky Route we have to 30,000 years light in the direction of the constellation of Sagittarius. Cygnus culminates during the nights of July and August in the meridian or zenith in northern hemisfere where it turns out impressive to observe in nights very dark and moved away of the urban centers the Milky Way or also denominated in the Average Age in Europe like the Way of Santiago, Christian peregrination to the city santa of Santiago de Compostela that is in Spain.
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| Main stars Alpha, a; denominated Deneb that means in Arab the tail of oca. of magnitude 1.33 it is a white supergiant that is to 3,200 years light of us and 60,000 times greater than our Sun It is a spectacular supergiant. Beta, b; denominated Albireo of color orange and magnitude 3,08. it is located in the South end of the constellation, light of us is to 386 years forms a binary system whose secondary it has a 5.30 magnitude and blue color, both are perfectly observed its colors with any telescope. It turns out precious to see both shining stars and orbiting on if same. Gamma, g; denominated Sadr, of magnitude 2.30 and clear yellow color. Dista 543 years Earth light. Delta, d; of magnitude 3.0, white color, is to 135 years light. Other objects M 29; stellar cluster of magnitude 6.60 that is to 4,000 years light of us and has an age of 10 million years formed by 20 stars of the eighth magnitude. M 39; stellar cluster of magnitude 4.60, is to only 970 years light and has an age of 270 million years. of 31' of diameter arc. |
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Observations
by telescope
D O U B L E |
Nom: b | R.A.: 19h.29m. | Dec: 33º38' |
|
| Mag: 3.1, 5.4 | Sep.: 34" | P.A.: 54º | Nat:f | Spec.:K, B |
| AOC: 99 | DSC: 71 | D.D.S.: 00-April-1984 | ||

NOTE: One is in a zone, very very rich; he is precious double a visible one at first, one is b Cygni or Albireo; the identification of the colors is simple, the main one is orange, however, the secondary one is bluish, blue a smooth one, form a set to expectacular, is one of those doubles that make history, are slightly separated, unfolding itself without difficulty with the eyeglass of 50x, although without a doubt some, the best image is obtained placing an eyeglass of 200x. Vale the pain to spend centuries contemplating similar spectacle
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D O U B L E |
Nom:17c1 | R.A.: 19h.44m. | Dec: 33º38' |
|
| Mag: 5.1, 8.5 | Sep.: 26" | P.A.: 69º | Nat:? | Spec.:B, G |
| AOC: 100 | DSC: 72 | D.D.S.: 00-April-1984 | ||
D O U B L E |
Nom: S 2576 | R.A.: 19h.44m. | Dec: 33º29' |
|
| Mag: 8.3, 8.4 | Sep.: 1.9" | P.A.: 359º | Nat:O | Spec.:?, ? |
| AOC: 101 | DSC: 73 | D.D.S.: 00-April-1984 | ||


NOTE: 17X1: One is in a rich zone; there is a remarkable difference of magnitude between the components, the main one is bluish, however, the secondary one is yellow although the color of the secondary hill to identify it. It is one pretty double and simple, it is unfolded without difficulty with the eyeglass of 50x.
S
2576: One is to 20' of the previous double, is inprescindible the eyeglass of 200x to unfold it, profit not to identify the colors of both components due to the proximity of them, are oriented in sense north-south.![]()
D O U B L E |
Nom:S 2578 | R.A.: 19h.44m. | Dec: 35º58' |
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| Mag: 6.4, 7.2 | Sep.: 15" | P.A.: 124º | Nat:f | Spec.:A, K |
| AOC: 224 | DSC: 159 | D.D.S.: 20h.45m.(UT); 30-Sep.-1984 (prism) | ||

NOTE: One is in a very rich zone; there is a slight difference of magnitude between the components, are slightly separated, although certain it is that very little, it is unfolded without difficulty with the eyeglass of 50x.
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D O U B L E |
Nom:S 2534 | R.A.: 19h.26m. | Dec: 36º26' |
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| Mag: 7.9, 8.1 | Sep.: 7" | P.A.: 65º | Nat:f | Spec.:A, B |
| AOC: 225 | DSC: 160 | D.D.S.: 20h.50m.(UT); 30-Sep.-1984 (prism) | ||

NOTE: One is in a rich zone; there is a slight difference of magnitude between the components, are together, although it is unfolded without difficulty with 50x, although it is necessary to pay attention to it; I estimate white the main color of, and bluish the secondary one, although I am not absolutely safe due to the weakness of the components.
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D O U B L E |
Nom:S 46 App | R.A.: 19h.40m. | Dec: 50º24' |
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| Mag: 6.3,6.4 | Sep.: 40" | P.A.: 135º | Nat:? | Spec.:?,? |
| AOC: 226 | DSC: 161 | D.D.S.:20h.54m.(UT);30-Sep.-1984 (prism) | ||
D O U B L E |
Nom:16,c | R.A.: 19h.41m. | Dec: 50º24' |
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| Mag: 6.3,8.5 | Sep.: 38" | P.A.: 135º | Nat:f | Spec.:?,? |
| AOC: 227 | DSC:162 | D.D.S.: 20h.55m.(UT); 30-Sep.-1984 (prism) | ||
D O U B L E |
Nom: Not catalogue. | R.A.: 19h.43m. | Dec: 50º47' |
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| Mag: 8.0,10.0 | Sep.: 35" | P.A.: 90º | Nat:? | Spec.:?,? |
| AOC: 228 | DSC: 163 | D.D.S.: 20h.56m.(UT); 30-Sep.-1984 (prism) | ||
D O U B L E |
Nom: Not catalogue. | R.A.: 19h.43m. | Dec: 51101' |
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| Mag: 10.0,10.0 | Sep.: 40" | P.A.: 1301 | Nat:? | Spec.:M,G |
| AOC: 229 | DSC: 164 | D.D.S.: 20h.57m.(UT); 30-Sep.-1984 (prism) | ||

NOTE:S 4App: One is in a rich zone; there is a smallest difference of magnitude between the components of the double, are slightly separated, profit not to identify the colors, is unfolded without difficulty with the eyeglass of 50x.
16, c: One is to 15' to the west of the previous double; there is a remarkable difference of magnitude between the components, are also, slightly separated, although profit not to identify the colors due to the weakness of the components.
DSC 228: One is one catalogued double but not to identify it in the Sky Catalogue 2000.0; one is to 20' to the north of S 46 App; it is one unequal double of brightness, very weak and slightly separated components, like the previous ones are unfolded with 50x.
DSC 229: 4Ãpp is to 40' to the north of S; one is like the previous one another catalogued but not identified double in Sky Catalogue; the components are very weak, approximately of the tenth magnitude, is unfolded without difficulty with 50x
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P L A N E T A R Y N E B U L A E |
NGC:6826 | M:-- |
R.A.: 19h.43m. |
Dec: 50º24' |
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Mag:8.8 |
Dim:27"x24" | AOC: 230 | NCAO: 66 | ||
| D.D.S.: 21h.04m.(UT); 30-Sep.-1984 (prism) | |||||

NOTE: One is to 10' of the double S 46 App; it is quite difficult to identify due to the small thing that is and in addition to that it is in a very rich zone; it is observed as a blurred star, but nothing else.
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C L U S T E R |
NGC:6811 |
M:-- |
R.A.: 19h.37m. |
Dec: 46º27' |
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Mag:9.2 |
Dim:12' | AOC: 231 | NCAO: 67 | ||
| D.D.S.: 20h.10m.(UT); 30-Sep.-1984 (prism) | |||||
D O U B L E |
Nom:Not catalogue. | R.A.: 19h.42m. | Dec: 46º09' |
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| Mag: 7.0,8.0 | Sep.: 15" | P.A.: 280º | Nat:? | Spec.:?,? |
| AOC: 232 | DSC: 165 | D.D.S.: 21h.12m.(UT); 30-Sep.-1984 (prism) | ||
D O U B L E |
Nom:OS 187 | R.A.: 19h.41m. | Dec: 46º47' |
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| Mag: 8.0, 8.5, 9.0 | Sep.(AB): 10" Sep.(AC): 20" |
P.A.(AB): 45º P.A.(AC): 100º |
Nat(AB):? Nat(AC): ? |
Spec.:A, B, B |
| AOC: 233 | DSC: 166 | D.D.S.: 21H.13M.(UT); 30-Sep.-1984 (prism) | ||

NOTE: NGC 6811: One is in a rich zone; it is a pretty stellar cluster, has form of ring, story twenty stars of the same magnitude; PC is to 900, is very little concentrated towards the center, the phantom of the youngest star is A0 and has an age of 540 million years.
DSC165: One is to 20' to the SSE of NGC6811; is one double catalogued but not identified in the Sky Catalogue 2000.0; there is a slight difference of magnitude, are ligermente separated, is unfolded with 50x.
OS 187: One is a triple to 15' to the west; it is formed by very weak of uncertain colors and slightly separated components unfolding itself without difficulty with the eyeglass of 50x.
The set in himself is very pretty with a precious stellar cluster and two precious doubles surrounding it.
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C L U S T E R |
NGC:6866 |
M:-- |
R.A.: 20h.02m. |
Dec: 43º51' |
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Mag: 9.0 |
Dim:6'x2' | AOC: 234 | NCAO: 68 | ||
| D.D.S.:21h.16m.(UT); 30-Sep.-1984 (prism) | |||||
D O U B L E |
Nom: h 1468 | R.A.: 20h.01m. | Dec: 40º18' |
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| Mag: 7.8, 8.8 | Sep.: 13.0" | P.A.: 279º | Nat: ? | Spec.: A, ? |
| AOC: 235 | DSC: 167 | D.D.S.:21h.18m.(UT); 30-Sep.-1984 (prism) | ||
D O U B L E |
Nom:OSS 196 | R.A.: 20h.01m. | Dec: 40º52' |
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| Mag: 7.0, 9.6 | Sep.: 55.2" | P.A.: 168º | Nat:? | Spec.:A, ? |
| AOC: 236 | DSC: 168 | D.D.S.: 21h.20m.(UT); 30-Sep.-1984 (prism) | ||

NOTE: NGC 6866: One is in a rich zone; it is formed by twenty stars, is a pretty stellar cluster oriented in an angle of 0ºó 180º. Parsecs is to 1,200, and has an age of 230 million years.
h 1468: One double is to 5' to the west of NGC6866 is catalogued and identified in the Sky Catalogue; it is formed by two stars of the same magnitude, are slightly separated, is unfolded without difficulty with the eyeglass of 50x.
OSS196: One is to 10' to the NGC6866 south; it is formed by two stars of very different considerable magnitude in eleven, are slightly separated, is unfolded without difficulty with the eyeglass of 50x. The set in himself, is very pretty and peculiar.
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D O U B L E |
Nom:b pm | R.A.: 19h.42m. | Dec: 40º02' |
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| Mag: 7.9, 7.9 | Sep.: 102.1" | P.A.: 165º | Nat:? | Spec.:A, ? |
| AOC:237 | DSC: 169 | D.D.S.:21h.33m.(UT); 30-Sep.-1984 (prism) | ||
C L U S T E R |
NGC:6819 |
M:-- |
R.A.: 19h.39m. |
Dec: 40º08' |
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Mag:9.0 |
Dim:7' | AOC: 238 | NCAO: 69 | ||
| D.D.S.: 21h.35m.(UT); 30-Sep.-1984 (prism) | |||||
D O U B L E |
Nom: Not catalogue. | R.A.: 19h.39m. | Dec: 40º08' |
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| Mag: 9.0,10.0 | Sep.: 12" | P.A.: 330º | Nat:? | Spec.:?,? |
| AOC: 239 | DSC: 170 | D.D.S.: 21h.39m.(UT); 30-Sep.-1984 (prism) | ||

NOTE: b p.m.: One is another catalogued and identified double in the Sky Catalogue; their components are very weak, are very separated almost 1'; profit not to identify it the colors, is unfolded without difficulty with the eyeglass of 50x.
NGC 6819: Cluster deals with pretty stellar, very small, observes totally granulated, for that reason it is impossible to count the number of stars of which it comprises of the cluster, it is to 2,200 PC, and it has an age of 3,500 million years.
DSC170: Double catalogued but not identified, of very weak and slightly separated components unfolding itself with 50x; profit not to identify it colors by the weakness of brightness of the components.
The set formed by a stellar cluster very granulated and two doubles. He is very pretty and peculiar. In addition it is necessary to add that all it is in a very rich zone
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D O U B L E |
Nom:S 2486 | R.A.: 19h.11m. | Dec: 49º45' |
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| Mag: 6.5,6.7 | Sep.: 8" | P.A.: 210º | Nat:ph | Spec.:G,G |
| AOC: 240 | DSC: 171 | D.D.S.: 21h.37m.(UT); 30-Sep.-1984 (prism) | ||

NOTE: One is one very pretty double; it is one double brilliant, easy to locate, and with a small difference of magnitude between the components, something is together although it is unfolded with 50x; I have the impression that both are yellow, although am not absolutely safe.
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D O U B L E |
Nom: y | R.A.: 19h.54m. | Dec: 52º18' |
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| Mag: 5.0,7.6 | Sep.: 3.6" | P.A.: 176º | Nat:ph | Spec.:K,K |
| AOC: 241 | DSC: 172 | D.D.S.: 21h.44m.(UT); 30-Sep.-1984 (prism) | ||

NOTE: One is in a somewhat rich zone; it is one double brilliant, easy to identify, both components are together being needed 200x to unfold it, I believe that both components are orange, is one pretty double
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D O U B L E |
Nom:S 2671 | R.A.: 20h.17m. | Dec: 55º14' |
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| Mag: 6.0,7.5 | Sep.: 3.6" | P.A.: 336º | Nat:ph | Spec.:B,B |
| AOC: 242 | DSC: 173 | D.D.S.:21h.55m.(UT); 30-Sep.-1984 (prism) | ||

NOTE: One is in a rich zone; something difficult to identify is unfolded with the eyeglass of 100x, since they are very together, is one very pretty double.
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C L U S T E R |
NGC:6996 |
M:-- |
R.A.: 20h.54m. |
Dec: 44º28' |
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Mag:9.4 |
Dim:16' | AOC: 321 | NCAO: 89 | ||
| D.D.S.: 22h.07m.(UT); 17-June-1985 | |||||

NOTE: One is in a rich zone; it is a weak stellar cluster, granulated, dark and pretty, is located to 500 PC.
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C L U S T E R |
NGC:6991 |
M:-- |
R.A.: 20h.54m. |
Dec: 47º16' |
|
Mag: 8.9 |
Dim:25' | AOC: 322 | NCAO: 90 | ||
| D.D.S.:22h.15m.(UT); 17-June-1985 | |||||
D O U B L E |
Nom:59 | R.A.: 20h.58m. | Dec: 47º20' |
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| Mag: 4.0, 9.2 | Sep.: 20" | P.A.: 353º | Nat:? | Spec.:A,B |
| AOC: 323 | DSC: 233 | D.D.S.:22h.21m.(UT); 17-June-1985 | ||

NOTE: NGC 6991: One is a small stellar cluster located in a rich zone; it is an cluster shining, and pretty, story approximately ten stars oriented in sense north-south.
59: One is to 30' to the NGC6991 west, is a remarkable difference of magnitude between the components, is one pretty double and delicate, it is unfolded without difficulty with the eyeglass of 50x, the main one I believe that she is white, however, the secondary one is bluish.
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C L U S T E R |
NGC:7039 |
M:-- |
R.A.: 21h.10m. |
Dec: 45º33' |
|
Mag:7.0 |
Dim:40'x25' | AOC: 324 | NCAO: 91 | ||
| D.D.S.:22h.32m.(UT); 17-June-1985 | |||||

NOTE: One is in a zone, very very rich; he is precious, a shining one and simple stellar cluster, the observed direction is of sense north-south, they are distinguished and they appeared signalized several shining stars. That they emphasize on the others. One is located to 1400 PC, and has an age of 1600 million years.
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C L U S T E R |
NGC:7082 |
M:-- |
R.A.: 21h.27m. |
Dec: 46º55' |
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Mag:9.5 |
Dim:20'x20' | AOC: 325 | NCAO: 92 | ||
| D.D.S.: 22h.42m.(UT); 17-June-1985 | |||||

NOTE: One is in a very rich zone; it is a shining cluster, story twenty stars without given direction. Is located to 1400 parsec, and has an age of about 1600 million years.
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C L U S T E R |
NGC:7092 |
M: 39 |
R.A.: 21h.30m. |
Dec: 48º13' |
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Mag:5.2 |
Dim:25' | AOC: 326 | NCAO: 93 | ||
| D.D.S.:22h.36m.(UT); 17-June-1985 | |||||

NOTE: One is in a rich zone; it is a shining, great, rich cluster stellar and very pretty, parsecs is to single 270, has an age of only 270 million years, very young; the phantom of the youngest star is A0, is formed by 30 stars.
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C L U S T E R |
NGC:7086 |
M:-- |
R.A.: 21h.28m. |
Dec: 51º25' |
|
Mag:9.5 |
Dim:7' | AOC: 327 | NCAO: 94 | ||
| D.D.S.: 21h.33m.(UT); 21-June-1985 | |||||

NOTE: One is in a very rich zone; it is observed totally granulated, in nebular form, is something difficult his identification, is small, dark. Is located to 1200 parsecs, has an age of 85 million years, the star with the youngest phantom is of the A5 type.
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C L U S T E R |
IC:5154 |
M:-- |
R.A.: 21h.51m. |
Dec: 47º02' |
|
Mag:10.5 |
Dim:12' | AOC: 328 | NCAO: 95 | ||
| D.D.S.:21h.39m.(UT); 20-June-1985 | |||||

NOTE: One is in a very rich zone; it is observed totally granulated, in nebular form, is something difficult his identification, he is small, shining and subtle. Is located to 1000 parsecs, has an age of 230 million years, the star with the youngest phantom is of the B1 type, has been nebular condensation due to its youth, is the famous Cocoon nebula. it is a nebula of pretty and, elliptical shining emission and amorphous and filamentous structure.
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| D O U B L E | Nom: OS 214 | R.A.: 21h.02m. | Dec: 41º26' | ||
| Mag: 6.4,8.7 | Sep.: 57" | P.A.: 184º | Nat:? | Spec.:B,F | |
| AOC: 330 | DSC: 235 | D.D.S.:21h.51m.(UT); 20-June-1985 | |||

NOTE: One is in a zone not very rich; there is a great difference of magnitude, are very separated, his colors are similarities, B and F; it is distinguished without difficulty with the eyeglass of 50x.
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D O U B L E |
Nom:61 | R.A.: 21h.04m. | Dec: 38º28' |
|
| Mag: 5.6,6.3 | Sep.: 29" | P.A.: 146º | Nat:O | Spec.:K,K |
| AOC: 331 | DSC: 236 | D.D.S.: 21h.55m.(UT); 20-June-1985 | ||

NOTE: One is in a rich zone; there is a small difference of magnitude, the separation is ideal, his colors are identified, she is pretty, it is distinguished with the eyeglass of 50x.
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C L U S T E R |
NGC:7063 |
M:-- |
R.A.: 21h.22m. |
Dec: 36º16' |
|
Mag:9.1 |
Dim:6' | AOC: 332 | NCAO: 96 | ||
| D.D.S.: 22h.01m.(UT); 20-June-1985 | |||||

NOTE: One is in a rich zone; it is a shining stellar cluster very easy to locate of small dimensions, very pretty, is located to 660 parsecs, it has an age of only 140 million years with a B8 phantom corresponding to the youngest star pertaining to the cluster formed by twelve stars.
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D O U B L E |
Nom:OS 437 | R.A.: 21h.18m. | Dec: 32º15' |
|
| Mag: 6.9,7.5 | Sep.: 2.2" | P.A.: 28º | Nat:ph? | Spec.:K,K |
| AOC: 333 | DSC: 237 | D.D.S.:22h.05m.(UT); 20-June-1985 | ||

NOTE: One is in a very rich zone; there is a smallest difference of magnitude, are together, both components are orange, is unfolded without difficulty with the eyeglass of 50x.
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D O U B L E |
Nom:S 2762 | R.A.: 21h.06m. | Dec: 30º00' |
|
| Mag: 5.7, 7.7, 9.0 | Sep.(AB): 3.4" Sep.(AC): 58" |
P.A.(AB): 306º P.A.(AC): 227º |
Nat(AB):? Nat(AC): op? |
Spec.:K, K, A |
| AOC: 334 | DSC: 238 | D.D.S.:22h.12m.(UT); 20-June-1985 | ||

NOTE: There is a small difference of magnitude in component AB; they are very together, unfolds with the eyeglass of 100x. Existe a great difference of magnitude between components BC, are very separated, the main one and the secondary one they are orange, however, the tertiary one is white, unfolds component BC with 50x.
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D O U B L E |
Nom:49 | R.A.: 20h.39m. | Dec: 32º08' |
|
| Mag: 6.0, 8.4 | Sep.: 2.8" | P.A.: 48º | Nat:f | Spec.:A, A |
| AOC: 335 | DSC: 239 | D.D.S.: 22h.34m.(UT); 20-June-1985 | ||

NOTE: There is a great difference of magnitude between the components, are very, very together, both components are white, is unfolded with 100x but with difficulty.
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D O U B L E |
Nom:S 2700 | R.A.: 20h.33m. | Dec: 32º20' |
|
| Mag: 6.8, 8.6 | Sep.: 24" | P.A.: 283º | Nat:f | Spec.:A, A |
| AOC: 336 | DSC: 240 | D.D.S.:22h.57m.(UT); 20-June-1985 | ||

NOTE: One is in a zone, very very rich; there is an appreciable difference of magnitude, are very separated, is unfolded without difficulty with the eyeglass of 50x, both components are white.
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D O U B L E |
Nom:S 2705 | R.A.: 20h.35m. | Dec: 33º11' |
|
| Mag: 7.3, 8.5 | Sep.: 3.1" | P.A.: 262º | Nat:f | Spec.:A, A |
| AOC: 337 | DSC: 241 | D.D.S.: 23h.03m.(UT); 20-June-1985 | ||

NOTE: One is in a rich zone; there is a slight difference of magnitude, are very together, both components are white, is unfolded with difficulty with the eyeglass of 100x.
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D O U B L E |
Nom:S 2708 | R.A.: 20h.37m. | Dec: 38º28' |
|
| Mag: 6.8, 8.5 | Sep.: 31" | P.A.: 315º | Nat:? | Spec.:A, B |
| AOC: 339 | DSC: 242 | D.D.S.: 23h.10m.(UT); 20-June-1985 | ||

NOTE: One is in a very rich zone; there is a great difference of magnitude between the components, are separated, is unfolded without difficulty with the eyeglass of 50x, the main one I see it blue, however, the secondary white.
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D O U B L E |
Nom:OS 414 | R.A.: 20h.45m. | Dec: 42º13' |
|
| Mag: 7.4, 8.7 | Sep.: 10" | P.A.: 94º | Nat:f | Spec.:A, B |
| AOC: 339 | DSC: 243 | D.D.S.:23h.14m.(UT); 20-June-1985 | ||

NOTE: One is in a zone, very, very very rich; there is a slight difference of magnitude between the components, are slightly together, is unfolded without difficulty with the eyeglass of 50x, the main one is bluish and the secondary white.
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C L U S T E R |
NGC:6910 |
M:-- |
R.A.: 20h.21m. |
Dec: 40º37' |
|
Mag:6.7 |
Dim:10'x5' | AOC: 340 | NCAO: 97 | ||
| D.D.S.: 23h.23m.(UT); 20-June-1985 | |||||

NOTE: One is in a zone, very very rich; it is a precious stellar, delicate, pretty cluster and shining, it is identified easily since cygni is to 40' to the south of g, the stars most shining of the field come signalized; parsecs is to 1650, has ten million years solely, with the youngest phantom of the type Or8, have been observed component the nebular environs of cluster along with g, are formed by 50 stars, the nebula is very opaque and invisible with the R-90mm., it is to irrregular amorphous and filamentous, it is of emission, sensible to the plates, and red.
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D O U B L E |
Nom:S 2666 | R.A.: 20h.16m. | Dec: 40º34' |
|
| Mag: 5.7, 8.1 | Sep.: 2.8" | P.A.: 245º | Nat:f | Spec.:A, B |
| AOC: 341 | DSC: 244 | D.D.S.:23h.35m.(UT); 20-June-1985 | ||

NNOTE: Very rich is in a zone; there is a great difference of magnitude, are very together, is unfolded with 100x, the main one is white and secondary the bluish one.
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C L U S T E R |
NGC:6913 |
M:29 |
R.A.: 20h.24m. |
Dec: 38º21' |
|
Mag:7.1 |
Dim:10'x8' | AOC: 342 | NCAO: 98 | ||
| D.D.S.: 23h.43m.(UT); 20-June-1985 | |||||
D O U B L E |
Nom: Dem 22 | R.A.: 20h.25m. | Dec: 40º14' |
|
| Mag: 8.1, 9.2 | Sep.: 3.1" | P.A.: 155º | Nat:? | Spec.: G, A |
| AOC: 343 | DSC: 245 | D.D.S.:23h.45m.(UT); 20-June-1985 | ||

NOTE: M29: Very richin stars is in a zone; it is a shining, small cluster stellar pretty and rich story thirty stars, the cluster is formed by fifty stars; is located to 1250 parsecs, has an age of only ten million years with a phantom corresponding to the youngest star of B0, has nebular, invisible condensation with the R-90 mm.
Dem 22: One is one catalogued and identified double in the Sky Catalogue 2000.0; their components are very weak, it is located to 20' to the south of M29, and it is unfolded with the eyeglass of 50x.
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C L U S T E R |
IC:4996 |
M:-- |
R.A.: 20h.15m. |
Dec: 37º24' |
|
Mag: 7.2 |
Dim:6' | AOC: 344 | NCAO: 99 | ||
| D.D.S.: 23h.55m.(UT); 20-June-1985 | |||||

NOTE:Very rich is in a zone; it is a shining cluster, something small, rich and pretty, one is to 1650 PC, he is very rich, it has cloudiness, it has a considered age of 10 million years, the phantom of the youngest star pertaining to the cluster is B0.
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C L U S T E R |
NGC:6883 |
M:-- |
R.A.: 20h.09m. |
Dec: 35º42' |
|
Mag: 7.8 |
Dim:25'x15' | AOC: 345 | NCAO: 100 | ||
| D.D.S.:00h.15m.(UT); 21-June-1985 | |||||

NOTE: Very rich is in a zone, is a shining, small, pretty cluster stellar and not very rich, parsecs is located to 1380, has an age of 15 million years and has nebular condensation.
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C L U S T E R |
NGC:6871 |
M:-- |
R.A.: 20h.04m. |
Dec: 35º38' |
|
Mag:5.6 |
Dim:37' | AOC: 346 | NCAO: 101 | ||
| D.D.S.:00h.20m.(UT); 21-June-1985 (prism) | |||||
D O U B L E |
Nom:S 2639 | R.A.: 20h.07m. | Dec: 35º20' |
|
| Mag: 7.6, 8.5 | Sep.: 5.8" | P.A.: 301º | Nat:f | Spec.:A, K |
| AOC: 347 | DSC: 246 | D.D.S.:00h.27m.(UT); 21-June-1985 (prism) | ||

NOTE: NGC 6871: Very richis in a zone, is great and rich a stellar cluster bonto,; parsecs is located to 1650, has an approximated age of only 10 million years; the phantom of the youngest star is Or6, nebular presence has been observed.
S 2639:
One is immersed in NGC 2671; there is a slight difference of magnitude, are together, although it is unfolded with 50x, the main one is white, however, the secondary one is orange.![]()
D O U B L E |
Nom: S 738 | R.A.: 20h.11m. | Dec: 33º38' |
|
| Mag: 8.6, 8.7 | Sep.: 41" | P.A.: 108º | Nat:? | Spec.:A, A |
| AOC: 348 | DSC: 247 | D.D.S.:00h.31m.(UT); 21-June-1985 (prism) | ||
D O U B L E |
Nom: h 1485 | R.A.: 20h.09m. | Dec: 33º25' |
|
| Mag: 8.3, 9.0 | Sep.: 4.7" | P.A.: 277º | Nat:? | Spec.:A, K |
| AOC: 349 | DSC: 248 | D.D.S.: 00h.35m.(UT); 21-June-1985 (prism) | ||

NOTE: S 738: One is in a rich zone; there is a smallest difference of magnitude between the components, are algos separated, both I see white them, is unfolded with 50x.
h 1485: One is another catalogued and found double in Sky Catalogue 2000.0; there is a remarkable difference of magnitude between the components, are something separated, the main one I see white it, however, secondary the orange, is to 20' to the northwest of S 708.
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D O U B L E |
Nom:OS 205 | R.A.: 20h.21m. | Dec: 41º00' |
|
| Mag: 7.0, 8.9 | Sep.: 45" | P.A.: 317º | Nat:? | Spec.:A, M |
| AOC: 358 | DSC: 253 | D.D.S.:21h.53m.(UT); 23-June-1985 | ||

NOTE: Very richin stars is in a field, is a remarkable difference of magnitude, are separated, the secondary one has a peculiar color rozijo, is unfolded without difficulty with 50x.
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C L U S T E R |
NGC:6834 |
M:-- |
R.A.: 19h.50m. |
Dec: 29º17' |
|
Mag:10.3 |
Dim:6'x3' | AOC: 359 | NCAO: 106 | ||
| D.D.S.: 22h.05m.(UT); 23-June-1985 | |||||

NOTE: Very richis in a field; it is a stellar cluster not very shining, of small dimensions in sense E-W, is luminous, precious. PC is located to 2300, and has an age of 70 million years
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D O U B L E |
Nom:52 | R.A.: 20h.44m. | Dec: 30º32' |
|
| Mag: 4.0, 9.2 | Sep.: 6.0" | P.A.: 69º | Nat:ph | Spec.:A, ? |
| AOC: 615 | DSC: 430 | D.D.S.:22h.05m.(UT); 01-July-1986 | ||

NOTE: Very richis in a zone; there is a great difference of magnitude, are very united, the main one is white, however, secondary the profit not to identify it, is unfolded with 100x.
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D O U B L E |
Nom:Arg 93 | R.A.: 20h.45m. | Dec: 32º41' |
|
| Mag: 8.9, 9.7 | Sep.: 11" | P.A.: 88º | Nat:f | Spec.:?, ? |
| AOC: 616 | DSC: 431 | D.D.S.: 22kh.17m.(UT); 1-July-1986 | ||

NOTE: Very rich is in a zone; there is a slight difference of magnitude, is one weak double of brightness of the components thus has been to me impossible to identify the colors, the identification is something difficult by the wealth of the field, is unfolded with 50x.
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D O U B L E |
Nom:Es | R.A.: 20h.41m. | Dec: 44º45' |
|
| Mag: 9.0, 9.5 | Sep.: 41" | P.A.: 297º | Nat:f' | Spec.:?, ? |
| AOC: 617 | DSC: 432 | D.D.S.: 22h.22m.(UT); 1-July-1986 | ||

NOTE: One is in a very rich zone; there is a slight difference of magnitude, are little separated, I do not identify the colors of his components, it is difficult to identify it due to the brightness weakness, and to the rich field, it is unfolded without difficulty with the eyeglass of 50x.
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D O U B L E |
Nom:S 2538 | R.A.: 19h.29m. | Dec: 36º36' |
|
| Mag: 8.6, 8.9, 9.0 | Sep.(AB): 6.0" Sep.(AC): 53" |
P.A.(AB): 51º P.A.(AC): 66º |
Nat(AB):f Nat(AC):f? |
Spec.:K, A, K |
| AOC: 804 | DSC: 599 | D.D.S.:21h.35m.(UT); 18-June-1987 | ||

NOTE: One is in a precious stellar field; there is a slight difference of magnitude between the three components, the main one and the tertiary one is orange, however, the secondary one is white, the separation is desproporcional, although it is unfolded without difficulty with 50x.
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D O U B L E |
Nom:OS 187 | R.A.: 19h.34m. | Dec: 46º20' |
|
| Mag: 8.3, 9.0, 9.0 | Sep.(AB): 64" Sep.(AC): 129" |
P.A.(AB): 287º P.A.(AC): 255º |
Nat(AB): op Nat(AC): op |
Spec.:?, ?, ? |
| AOC: 810 | DSC: 605 | D.D.S.:22h.20m.(UT); 18-June-1987 | ||

NOTE: One is in a rich field; there is a slight difference of magnitude between components AB and equality in BC, as much B is very separated as C of A; profit not to identify the colors due to the weakness of the components, is unfolded without difficulty with the eyeglass of 50x.
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D O U B L E |
Nom:OS 379 | R.A.: 19h.36m. | Dec: 33º46' |
|
| Mag: 8.0, 9.4 | Sep.: 25" | P.A.: 86º | Nat:f | Spec.:A, B |
| AOC:811 | DSC: 606 | D.D.S.: 22h.29m.(UT); 18-June-1987 | ||

NOTE: One is in a very rich zone; there is a remarkable difference of magnitude, are slightly separated, is unfolded without difficulty with the eyeglass of 50x, the main one is white, however, the secondary one is bluish, is one pretty double.
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D O U B L E |
Nom: d | R.A.: 19h.43m. | Dec: 45º00' |
|
| Mag: 2.9, 6.3 | Sep.: 2.2" | P.A.: 232º | Nat:O | Spec.:A, A |
| AOC: 812 | DSC: 607 | D.D.S.:22h.39m.(UT); 18-June-1987 | ||

NOTE: One is in a partially rich zone; there is a remarkable difference of magnitude, are very together, I need 200x to unfold it, is one very pretty but out of proportion double; both components are white.
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constellations
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Masm (Last update 2004-02-21)