Документ взят из кэша поисковой машины. Адрес
оригинального документа
: http://www.stsci.edu/~inr/pmsu/tab1bs.html
Дата изменения: Fri Jun 8 23:32:03 2007 Дата индексирования: Tue Oct 2 04:46:07 2012 Кодировка: Поисковые слова: р п р р п п р п п р п п р п п р п п р п п р п п р п п р п п р п п р п |
Positions. distances and estimated absolute magnitudes for southern (dec < -30o)
late-type binary companions
listed in pCNS3. All of these stars were too close to the primary to allow observation
as part of the PMSU. The format of this table is similar to Table 1A, save that the position
and distance information are for the primary star in the system. Positions are taken from the
following sources:
1. Co-ordinates measured at the Palomar 60-inch telescope
2. Co-ordinates measured at either the Palomar 200-inch telescope, Keck or the AAT
3. HST Guide Star catalogue (version 1)
4. pCNS3
5. Digital Sky Survey images
6. Hipparcos
Column 9 lists the apparent magnitude of the primary, column 10, the estimated magnitude
difference (at V), and column 11, the separation, in arcseconds. Column 12 gives the
contribution from parallax data to the distance estimate - see Table 1A for coding.
NN | Name | RA (2000) | Dec | Ref | MV | Dist (pc) | % d | VP | dV | rho | ftrig | |
---|---|---|---|---|---|---|---|---|---|---|---|---|
292 | Gl 60 C | 1: 35: 0.7 | -29: 54: 39 | 3 | 8.54 | 13.6 | 6 | 7.8 | 1.6 | 1.4 | 105 | . |
345 | Gl 81 B | 1: 54: 4.2 | -51: 51: 9 | 3 | 9.30 | 17.5 | 1 | 3.7 | 2.4 | 5.0 | 105 | . |
368 | Gl 83.4B | 2: 3: 54.9 | -45: 24: 47 | 6 | 8.00 | 49.2 | 5 | 7.3 | 4.2 | 1.6 | 105 | . |
1002 | Gl 225.2B | 6: 0: 19.8 | -31: 1: 52 | 6 | 7.63 | 19.7 | 29 | 8.3 | 0.8 | 0.9 | 51 | . |
1111 | Gl 257 B | 6: 57: 47.5 | -44: 17: 27 | 6 | 12.18 | 8.0 | 2 | 11.5 | 11.7 | 0.2 | 105 | . |
1261 | Gl 294 C | 7: 57: 3.0 | -60: 9: 2 | 3 | 12.45 | 16.2 | 0 | 9.9 | 9.1 | 2.3 | 105 | . |
1301 | -35 4406B | 8: 14: 19.0 | -35: 43: 5 | 3 | 10.30 | 14.3 | 17 | 7.2 | 6.5 | 2.5 | 0 | . |
1549 | Gl 368.1B | 9: 47: 0.7 | -52: 22: 24 | 3 | 10.20 | 26.2 | 2 | 7.9 | 6.2 | 1.4 | 105 | . |
1590 | Gl 379.1B | 10: 7: 20.4 | -35: 36: 30 | 3 | 8.42 | 30.7 | 1 | 6.2 | 4.5 | 2.5 | 105 | . |
3413 | *LTT8708 B | 21: 49: 10.7 | -41: 33: 24 | 3 | 11.73 | 17.5 | 14 | 12.9 | 11.7 | 1.0 | 0 | . |
3507 | Gl 853 B | 22: 15: 2.2 | -53: 52: 6 | 3 | 9.23 | 13.6 | 0 | 5.4 | 5.0 | 0.0 | 105 | . |
3803 | GJ 1294 B | 0: 2: 8.4 | -68: 16: 48 | 6 | 9.60 | 15.9 | 3 | 9.7 | 8.6 | 1.5 | 105 | . |
Gl - Gliese (1969); GJ - Gliese & Jahreiss (1979); Wo - Woolley et al, (1970); LHS - Luyten Half-Second Catalogue; LTT - Luyten Two-Tenths Catalogue; LP - Luyten Palomar proper-motion catalogue; G - Giclas et al (1971); GR - Giclas et al (1971) red star; GH - Giclas et al (1971) Hyades star; Rob - Robertson (1984); Steph - Stephenson (1986); PS - Pesch & Sanduleak (1978); San - Sanduleak (1976); vA - van Altena (1969); V - Vyssotsky (1963)
Neill Reid - last revised23 June, 2001