1986NIA86......193D


C.D.S. - SIMBAD4 rel 1.7 - 2021.04.15CEST12:14:52

1986NIA86......193D - New insights in astrophysics. Proc. International Symp. co-sponsored by NASA, ESA and SERC, held at Univ. Coll. London, 14-16 July 1986. ESA SP-263, 193-196 (1986)

The stellar winds of K and early M giants : evidence for a subclass with abnormally high expansion velocities.

DRAKE S.A.

Journal keyword(s):

Simbad objects: 16

goto View the reference in ADS

Number of rows : 16

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2021
#notes
1 * del And SB* 00 39 19.6751809 +30 51 39.678320 6.04 4.56 3.28 2.36 1.70 K3III-IIIbCN0.5 316 0
2 * eta Cet HB* 01 08 35.3914827 -10 10 56.156955 5.80 4.61 3.45 2.61 2.03 K2-IIIb 202 0
3 * gam Phe SB* 01 28 21.9272669 -43 19 05.650173   4.98 3.41     M0III 136 0
4 * alf Cet LP? 03 02 16.77307 +04 05 23.0596 6.10 4.17 2.53 1.18 0.02 M1.5IIIa 441 0
5 * tau04 Eri LP* 03 19 31.0022373 -21 45 28.304953 7.13 5.32 3.70 2.12 0.66 M3III-IIIaCa-1 105 0
6 * gam Eri LP? 03 58 01.7669489 -13 30 30.669770 6.52 4.54 2.94 1.68 0.68 M0III-IIIb 172 0
7 * bet Col PM* 05 50 57.5921991 -35 46 05.915211 5.49 4.28 3.12 2.27 1.69 K1III_CN+1 136 0
8 * sig Pup SB* 07 29 13.8304917 -43 18 05.159662 6.54 4.77 3.25 2.04 1.12 K5III 123 0
9 * bet Cnc PM* 08 16 30.9210081 +09 11 07.957924 6.750 5.000 3.520 2.42 1.62 K4IIIBa0.5: 346 0
10 * N Vel V* 09 31 13.3189137 -57 02 03.757780   4.691 3.139     K5III 90 0
11 * nu. Hya PM* 10 49 37.4887449 -16 11 37.135989 5.62 4.35 3.11 2.17 1.53 K1.5IIIHdel-0.5 160 0
12 * eps Cru PM* 12 21 21.6093625 -60 24 04.129070   5.01 3.59     K3III 84 0
13 * del Vir RG* 12 55 36.2086058 +03 23 50.893225 6.76 4.97 3.38 1.86 0.53 M3+III 260 0
14 * del Mus SB* 13 02 16.2647362 -71 32 55.875239   4.80 3.62     K2III 61 0
15 * rho Boo PM* 14 31 49.7896173 +30 22 17.178087 6.33 4.89 3.59 2.67 2.02 K3-III 248 0
16 * zet Ara * 16 58 37.2121689 -55 59 24.520302   4.701 3.076     K3III 90 0

    Equat.    Gal    SGal    Ecl

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2021.04.15-12:14:52

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