Документ взят из кэша поисковой машины. Адрес оригинального документа : http://lnfm1.sai.msu.ru/~anna/kinem-OB-ass.txt Дата изменения: Fri Mar 7 13:51:32 2003 Дата индексирования: Mon Oct 1 21:56:59 2012 Кодировка: Поисковые слова: http www.astronomy.ru forum index.php topic 4644.0.html

----------- The catalog of line-of-sight velocities -------------
---------- and proper motions of the OB-associations ------------

Notation

OB-ass. - the name of OB-association from C.Blaha and R.M.Humphreys
list (1989);

l - the mean galactic longitude;

b - the mean galactic latitude;

r - the mean heliocentric distance, which equals r=0.8 rBH,
where rBH is the mean heliocentric distance from Blaha and Humphreys'
catalog (1989), for more details see the paper by Dambis et al (2001);

Vr - the median line-of-sight velocity of the stars of the OB-association,
km/s;

dvr - the estimation of the line-of-sight velocity dispersion in
the OB-association, km/s;

nr - the number of stars in the OB-association with known line-of-sight
velocities, which were taken from the catalog of M.Barbier-Brossat and
P.Figon (2000); only velocities with estimation errors less than 10 km/s
were taken into account;

mul - the median proper motion along galactic longitude of the stars
of the OB-association, in units of 0.001 arcsec/year;

dml- the estimation of mul dispersion in the OB-association,
in 0.001 arcsec/year;

mub - the median proper motion along galactic latitude of the stars
of the OB-association, in units of 0.001 arcsec/year;

dmb- the estimation of mub dispersion in the OB-association,
in 0.001 arcsec/year;

nm - the number of stars of the OB-association with known proper motion
from HIPPARCOS catalog (1997).

Nt - the total number of stars in the OB-association
with known photometry from the catalog by Blaha and Humphreys (1989)

OB-ass. l b r Vr dvr nr mul dml mub dmb nm Nt
SGR OB5 0.0 -1.2 2.4 -15.0 19.0 2 0.1 1.7 0.1 2.2 3 31
SGR OB1 7.6 -0.8 1.3 -10.0 12.1 37 -1.6 1.2 -1.3 1.0 29 66
SGR OB7 10.7 -1.6 1.4 -6.1 17.1 3 -0.0 0.3 -3.3 0.1 2 4
SGR OB4 12.1 -1.0 1.9 3.5 10.8 9 -0.7 1.4 -0.8 2.5 3 15
SER OB1 16.7 0.1 1.5 -5.0 20.0 17 -0.7 0.9 -0.8 1.7 12 43
SCT OB3 17.3 -0.7 1.3 3.3 17.0 8 -0.9 0.5 -0.6 1.0 3 10
SER OB2 18.2 1.6 1.6 -4.0 14.5 7 -0.8 0.7 -1.4 0.2 5 18
SCT OB2 23.2 -0.5 1.6 -11.0 20.0 6 -0.5 2.8 -0.6 1.2 6 13
TR 35 28.0 -0.5 2.0 31.0 1 -3.2 -0.1 1 9
COLL 359 29.8 12.6 0.2 -7.2 -4.1 1 1
VUL OB1 60.4 0.0 1.6 3.1 14.7 9 -4.7 1.7 -0.1 0.7 8 28
VUL OB4 60.6 -1.2 0.8 -2.9 7.5 3 -4.1 1.1 -1.9 1.2 3 9
CYG OB3 72.8 2.0 1.8 -9.5 9.5 30 -7.6 0.9 -1.2 1.2 18 42
CYG OB1 75.8 1.1 1.5 -13.5 8.9 34 -6.3 1.0 -0.8 1.3 14 71
CYG OB9 77.8 1.8 1.0 -19.5 8.6 10 -6.7 1.5 -1.4 0.7 8 32
CYG OB8 77.9 3.4 1.8 -21.0 11.0 9 -6.2 0.5 0.8 1.1 10 21
CYG OB2 80.3 0.9 1.5 -3.9 -1.5 1 15
CYG OB4 82.7 -7.5 0.8 -4.9 1.1 2 -0.6 1.7 -1.3 1.5 2 2
CYG OB7 89.0 0.0 0.6 -9.4 9.3 21 -3.2 3.5 -1.1 1.2 28 29
NGC 6991 87.6 1.4 1.4 -15.0 1 -4.7 -0.3 1 1
LAC OB1 96.7 -17.7 0.5 -13.6 4.2 2 -3.4 0.2 -4.4 0.4 2 2
CEP OB2 102.1 4.6 0.7 -17.0 6.7 37 -3.9 1.3 -0.8 1.4 47 59
CEP OB1 104.2 -1.0 2.8 -58.2 7.4 17 -3.9 0.7 -0.4 0.9 24 58
NGC 7235 102.8 0.8 3.2 1
CAS OB2 112.0 0.0 2.1 -50.1 11.0 7 -4.5 1.0 -0.1 1.1 5 41
CEP OB3 110.4 2.6 0.7 -22.9 3.9 18 -2.2 1.3 -1.7 1.6 15 26
CAS OB5 116.1 -0.5 2.0 -45.8 7.2 16 -3.5 1.1 -2.0 1.2 13 52
CAS OB4 120.1 -0.3 2.3 -37.0 8.6 7 -2.1 1.2 -1.2 1.1 7 27
CAS OB14 120.4 0.7 0.9 -15.0 7.0 4 1.6 2.0 -1.1 1.1 3 8
CAS OB7 123.0 1.2 2.0 -50.0 3.0 4 -2.0 0.7 -0.9 0.7 8 39
CAS OB1 124.7 -1.7 2.0 -42.0 2.5 5 -2.0 0.0 -1.6 1.4 3 11
NGC 457 126.7 -4.4 2.0 -34.8 3.0 4 -1.7 0.2 -1.7 0.2 2 4
CAS OB8 129.2 -1.1 2.3 -34.7 9.9 14 -1.4 0.6 -1.0 1.9 9 43
PER OB1 134.7 -3.2 1.8 -43.4 7.0 81 0.1 1.0 -1.7 1.4 63 167
CAS OB6 135.0 0.8 1.8 -42.7 8.2 12 -0.5 1.4 -1.2 1.4 13 46
CAM OB1 141.1 0.9 0.8 -11.0 9.4 30 0.6 2.0 -1.7 1.6 33 50
CAM OB3 147.0 2.8 2.6 -27.6 19.3 3 1.6 2.1 0.9 0.9 3 8
PER OB3 146.6 -5.9 0.1 -2.4 1 34.5 -8.3 1 1
PER OB2 160.3 -16.5 0.3 21.2 4.5 7 6.5 2.4 -1.3 1.7 7 7
AUR OB1 173.9 0.1 1.1 -1.9 14.0 26 3.0 1.3 -2.0 1.9 20 36
ORI OB1 206.9 -17.7 0.4 25.4 7.9 62 0.7 1.3 0.6 1.9 59 70
AUR OB2 173.3 -0.2 2.4 -2.7 4.8 4 0.1 1.0 -0.9 0.1 2 20
NGC 1893 173.6 -1.7 2.9 10
GEM OB1 189.0 2.2 1.2 16.0 5.0 18 1.5 1.3 -1.1 1.0 17 40
MON OB1 202.1 1.1 0.6 23.4 13.0 7 1.9 1.8 -2.1 2.2 7 7
MON OB2 207.5 -1.6 1.2 22.3 12.5 26 -1.1 1.5 -1.2 1.6 18 32
MON OB3 217.6 -0.4 2.4 27.0 1 4
CMA OB1 224.6 -1.6 1.1 34.3 16.1 8 -3.2 0.6 -2.6 1.1 10 17
NGC 2414 231.1 1.0 3.2 67.2 1 -2.6 -0.4 1 15
COLL 121 238.5 -8.4 0.6 29.6 7.0 10 -5.2 1.2 -1.0 0.9 13 13
NGC 2362 237.9 -5.9 1.2 30.0 14.0 6 -4.2 1.5 0.1 0.9 3 9
PUP OB2 244.6 0.6 3.2 13
COLL 140 244.5 -7.3 0.3 10.3 6.6 5 -7.0 0.9 -5.3 1.8 6 6
PUP OB3 253.9 -0.3 1.5 3
VELA OB2 262.1 -8.5 0.4 24.0 9.7 13 -9.7 1.5 -1.5 1.9 12 13
VELA OB1 264.9 -1.4 1.5 23.0 4.4 18 -6.8 1.2 -1.3 0.9 18 46
CAR OB1 286.5 -0.5 2.0 -5.0 8.2 39 -7.6 0.5 -1.0 0.3 18 126
TR 16 287.3 -0.3 2.1 -1.0 3.3 5 -7.2 0.5 -1.0 0.1 2 18
TR 14 287.4 -0.5 2.8 -10.0 1 5
TR 15 287.6 -0.4 3.0 2
COLL 228 287.6 -1.0 2.0 -13.0 9.0 9 -6.7 0.7 -1.0 0.1 2 15
CAR OB2 290.4 0.1 1.8 -8.2 8.5 22 -6.8 0.8 -0.8 0.7 12 59
NGC 3576 291.3 -0.6 2.5 -17.0 9.0 2 5
CRU OB1 294.9 -1.1 2.0 -5.3 8.9 33 -6.0 1.0 -0.8 0.6 19 76
NGC 3766 294.1 -0.0 1.5 -15.6 0.7 2 -6.3 0.5 -0.9 0.1 2 12
CEN OB1 304.2 1.4 1.9 -19.0 14.5 32 -4.9 0.8 -0.9 0.9 32 103
HOGG 16 307.5 1.4 1.5 -35.0 8.5 3 -4.1 1.4 -2.6 2.9 3 5
R 80 309.4 -0.4 2.9 -38.2 1 -6.1 -2.4 1 2
NGC 5606 314.9 1.0 1.5 -37.8 1.8 3 -4.9 2.0 -1.8 0.3 2 5
CIR OB1 315.5 -2.8 2.0 4
PIS 20 320.4 -1.5 3.2 -49.0 1 -11.7 1.4 1 6
R 103 332.4 -0.8 3.2 -48.0 26.0 11 -3.9 0.5 -1.9 0.7 4 34
ARA OB1B 338.0 -0.9 2.8 -34.7 10.4 9 -3.7 0.6 -2.2 0.7 6 21
ARA OB1A 337.7 -0.9 1.1 -36.3 20.6 8 -2.5 1.2 -2.2 1.3 10 53
NGC 6204 338.3 -1.1 2.2 -51.0 5.8 5 14
SCO OB1 343.7 1.4 1.5 -28.8 15.3 28 -1.5 0.6 -0.7 0.6 16 76
SCO OB2 351.3 19.0 0.1 -4.1 2.3 10 -23.9 1.8 -8.7 2.1 10 10
HD 156154 351.3 1.4 2.1 -4.0 8.5 3 -1.2 0.1 -0.9 1.2 2 4
SCO OB4 352.7 3.2 1.0 3.0 6.3 7 -0.7 0.2 -2.3 0.5 4 11
TR 27 355.1 -0.7 0.9 -15.8 1 11
M 6 356.8 -0.9 0.4 -6.4 1 -6.7 -1.7 1 1