Telescopium (Tel)
Here is a listing of 25 double stars in Telescopium. Doubles which have stars that show colour are marked in shaded rows. The names of the stars contains a link to the Simbad entry for it, containing more information.
Name | Sep | PA | Mag1 | Mag2 | RA | Dec | Spect | Comments |
---|---|---|---|---|---|---|---|---|
B 1879 | 1.7 | 266 | 6.0 | 11.5 | 18:11.1 | -47:31 | K1 | |
HDO 288 | 1.8 | 149 | 7.0 | 10.5 | 18:12.9 | -50:34 | F0 | |
I 429 | 0.1 | 146 | 8.5 | 8.5 | 18:15.0 | -50:19 | A0 | |
HJ 5033 | 17.3 | 115 | 7.0 | 9.5 | 18:15.4 | -48:52 | K0 | Third component sep 18.2, pa 9 mag 11, fouth component sep 27.9, pa 64 mag 9.5 |
I 1361 | 2.6 | 254 | 7.5 | 12.0 | 18:20.3 | -49:07 | A2 | |
DUN 220 | 31.1 | 178 | 8.0 | 8.5 | 18:22.2 | -55:33 | G0 | |
HJ 5041 | 2.6 | 259 | 7.5 | 9.5 | 18:25.9 | -53:39 | F0 | |
HJ 5045 | 8.3 | 23 | 7.0 | 10.5 | 18:31.0 | -48:00 | G0 | |
HJ 5049 | 19.9 | 264 | 7.0 | 11.0 | 18:37.4 | -47:04 | F2 | |
HJ 5053 | 32.6 | 197 | 8.0 | 10.0 | 18:43.5 | -55:45 | F5 | Primary is also a very close double. Both mag 8, sep 0.2 |
I 112 | 1.6 | 186 | 7.5 | 9.5 | 18:54.0 | -47:17 | F5/A0 | Third component sep 84.0, pa 63 mag 7.5 |
I 113 | 2.6 | 227 | 6.5 | 10.0 | 18:58.9 | -48:29 | K5 | |
HJ 5100 | 19.4 | 152 | 7.0 | 12.0 | 19:18.7 | -56:08 | B5 | Very hot, very blue primary |
I 1397 | 1.5 | 336 | 6.5 | 11.0 | 19:19.6 | -51:34 | A0 | |
HJ 5114 | 69.0 | 254 | 5.5 | 7.0 | 19:27.8 | -54:19 | K2/G0 | Third component Sep 70.5, pa 96 mag 11. B is also a close double, sep 8.3, pa 195 mag 11 |
I 118 | 1.2 | 132 | 7.5 | 10.0 | 19:33.0 | -46:46 | G5 | |
COO 238 | 3.3 | 50 | 7.5 | 8.5 | 19:42.3 | -52:56 | A3 | |
HJ 5148 | 14.2 | 318 | 7.0 | 12.0 | 19:50.2 | -45:23 | K0 | |
DUN 227 | 22.9 | 149 | 6.0 | 6.5 | 19:52.7 | -54:58 | G5/A2 | |
FIN 31 | 1.8 | 54 | 8.0 | 12.5 | 19:55.0 | -51:48 | K0 | |
I 256 | 1.0 | 194 | 7.5 | 9.5 | 20:01.4 | -47:23 | K0 | |
I 123 | 8.2 | 184 | 7.0 | 11.0 | 20:10.7 | -46:44 | K0 | |
SEE 415 | 11.1 | 97 | 7.5 | 12.0 | 20:20.9 | -45:32 | F5 | |
HJ 5187 | 17.8 | 323 | 8.0 | 13.5 | 20:22.6 | -54:16 | K0 | |
I 664 | 1.0 | 280 | 8.0 | 9.0 | 20:29.1 | -51:04 | F0 |