2001ApJ...562L..87Z


Query : 2001ApJ...562L..87Z

2001ApJ...562L..87Z - Astrophys. J., 562, L87-L90 (2001/November-3)

The β Pictoris moving group.

ZUCKERMAN B., SONG I., BESSELL M.S. and WEBB R.A.

Abstract (from CDS):

Following the 1983 IRAS detection and subsequent imaging of its extensive dusty circumstellar disk, β Pictoris became the prototypical and most studied example of a potential forming planetary system. Here we report the identification of 17 star systems, each with one or more characteristics indicative of extreme youth, that are moving through space together with β Pic. This diverse set of ∼12 million yr old star systems, which includes a ∼35 Jupiter mass brown dwarf, and a wide assortment of dusty circumstellar disks, is the comoving, youthful group closest to Earth. Their unique combination of youth and proximity to Earth makes group members–many of which have masses similar to that of the Sun–prime candidates for imaging of warm planets and dusty circumstellar disks with ground- and space-based telescopes.

Abstract Copyright: ∼

Journal keyword(s): Galaxy: Open Clusters and Associations: Individual: Name: β Pictoris - Stars: Kinematics - Stars: Pre-Main-Sequence

Simbad objects: 29

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Number of rows : 29
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NAME Tuc Moving Group MGr 00 00 -64.0           ~ 73 0
2 HD 203 PM* 00 06 50.0863238088 -23 06 27.145662264   6.547 6.173   5.74 F3V 140 0
3 Cl Melotte 22 OpC 03 46 38.0 +24 10 41           ~ 3679 0
4 HD 23309 * 03 50 38.6803877136 +73 54 30.332720052   9.80 9.12     G0 15 0
5 * 51 Eri PM* 04 37 36.1326090888 -02 28 24.775726260   5.486 5.209     F0IV 285 0
6 StKM 1-497 TT* 04 37 37.4553491592 -02 29 28.950973764   12.04 10.59   8.59 M1.1V 138 0
7 CD-57 1054 PM* 05 00 47.1296589456 -57 15 25.452888732   11.36 9.977 9.889 8.177 M0Ve 143 0
8 V* AF Lep RS* 05 27 04.7633281608 -11 54 03.466002240   6.832 6.295     F8V(n)k: 285 0
9 * bet Pic PM* 05 47 17.0876901 -51 03 59.441135 4.13 4.03 3.86 3.74 3.58 A6V 2087 1
10 V* AO Men PM* 06 18 28.2078302088 -72 02 41.447954904   11.06 9.809 9.299 8.456 K4Ve 153 0
11 NAME TW Hya Association As* 11 01.9 -34 42           ~ 1018 0
12 NAME beta Pic Moving Group MGr 14 30 -42.0           ~ 894 0
13 HD 139084 SB* 15 38 57.5566916952 -57 42 27.346084668   8.78 7.977   7.106 K0V 174 0
14 * d Sco PM* 16 18 17.8991603537 -28 36 50.471996469   4.804 4.782     A1Va 172 0
15 HD 155555 RS* 17 17 25.5053342232 -66 57 03.732141636 7.795 7.499 6.723   6.39 G5V+K1V 292 1
16 HD 155555C Y*? 17 17 31.2882831192 -66 57 05.470945380   14.36 12.82 12.33   M3Ve 70 1
17 HD 164249 PM* 18 03 03.4097283792 -51 38 56.432149872   7.438 7.007 7.90   F6V 142 0
18 CD-43 12272A PM* 18 06 49.8929258688 -43 25 30.800909676   5.84 5.62     A6V 74 0
19 CD-43 12272 ** 18 06 49.89312 -43 25 30.7964   5.17 4.95     A6V+A7V 54 0
20 HD 172555 PM* 18 45 26.9009806435 -64 52 16.534807985   4.967 4.767     A7V 321 0
21 CD-64 1208 SB* 18 45 37.0492713148 -64 51 45.888646069   10.518 9.433 9.694   K5Ve 74 0
22 V* PZ Tel BY* 18 53 05.8735056984 -50 10 49.897437168   9.22 8.342   7.464 G9IV 364 0
23 * eta Tel PM* 19 22 51.2060774616 -54 25 26.145617376   5.035 5.020   4.99 A0V 228 0
24 * eta Tel B LM* 19 22 51.3580284238 -54 25 31.569876496           M7.5V 78 0
25 HD 181327 PM* 19 22 58.9437222504 -54 32 16.975668624   7.50 7.04   6.49 F6V 331 0
26 V* AT Mic Er* 20 41 51.15925 -32 26 06.8283 12.753 11.909 10.343 9.098 7.383 M4.5Ve+M4.5Ve 371 0
27 HD 197481 BY* 20 45 09.5324974119 -31 20 27.237889841   10.05 8.627 9.078 6.593 M1VeBa1 1344 0
28 HD 199143 PM* 20 55 47.6748292416 -17 06 51.061731768   7.84 7.32 8.29   F8V 133 0
29 HD 358623 BY* 20 56 02.738688 -17 10 53.80428   11.603 10.625 10.18 8.847 K7 103 0

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