2002ApJ...568..352V

Query : 2002ApJ...568..352V

2002ApJ...568..352V - Astrophys. J., 568, 352-362 (2002/March-3)

Ten low-mass companions from the Keck precision velocity survey.

VOGT S.S., BUTLER R.P., MARCY G.W., FISCHER D.A., POURBAIX D., APPS K. and LAUGHLIN G.

Abstract (from CDS):

Ten new companions have emerged from the Keck precision Doppler velocity survey, with minimum (Msini) masses ranging from 0.8 MJUP to 0.34 M☉. Five of these are planet candidates with Msini<12 MJUP, two are brown dwarf candidates with Msini∼30 MJUP, and three are low-mass stellar companions. Hipparcos astrometry reveals the orbital inclinations and masses for three of the (more massive) companions, and it provides upper limits to the masses for the rest. A new class of extrasolar planet is emerging, characterized by nearly circular orbits and orbital radii greater than 1 AU. The planet HD 4208b appears to be a member of this new class. The mass distribution of extrasolar planets continues to exhibit a rapid rise from 10 MJUP toward the lowest detectable masses near 1 MSAT.

Abstract Copyright: ∼

Journal keyword(s): Stars: Planetary Systems - Techniques: Radial Velocities

Simbad objects: 31

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Number of rows : 31
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024 		#notes
1 HD 4208 PM* 00 44 26.6506707202 -26 30 56.455527913   8.46 7.79     G7VFe-1CH-0.5 201 1
2 HD 4208b Pl 00 44 26.6506707202 -26 30 56.455527913           ~ 39 1
3 HD 4203b Pl 00 44 41.2002505536 +20 26 56.138079876           ~ 38 1
4 HD 4203 PM* 00 44 41.2002505536 +20 26 56.138079876       8.2   G6V 140 1
5 * ups And b Pl 01 36 47.8415443907 +41 24 19.651368029           ~ 272 1
6 * eps Ret PM* 04 16 29.0281470260 -59 18 07.755891304 6.59 5.52 4.44 3.62 3.08 K2III 238 1
7 HD 33636 Pe* 05 11 46.4494089528 +04 24 12.742146936   7.64   6.6   G0V_CH-0.3 190 1
8 HD 33636B LM* 05 11 46.45 +04 24 12.7           ~ 48 1
9 HD 35956 SB* 05 28 51.6281116200 +12 33 02.925812808 7.40 7.35 6.76 6.25 5.92 G0V 77 0
10 HD 43587 SB* 06 17 16.1297031648 +05 05 59.904745548 6.400 6.290   5.3   G0V 241 0
11 HD 46375 PM* 06 33 12.6224391648 +05 27 46.528531452   8.70 7.84     G9V 234 2
12 HD 64468 SB* 07 54 54.0653165265 +19 14 10.838142912 9.548 8.715 7.726 7.182 6.723 K2.5V 80 0
13 HD 68988 PM* 08 18 22.1728652088 +61 27 38.595044628   8.84 8.19     G1V 155 2
14 HD 68988b Pl 08 18 22.1728652088 +61 27 38.595044628           ~ 50 1
15 HD 75289 PM* 08 47 40.3893739728 -41 44 12.455319264 7.04 6.94 6.36     F9VFe+0.3 279 1
16 BD-10 3166 PM* 10 58 28.7841138528 -10 46 13.394735436   10.88 10.01 9.85 9.19 K3.0V 133 1
17 * 47 UMa PM* 10 59 27.9727514012 +40 25 48.920572724   5.66   4.7   G1-VFe-0.5 773 1
18 HD 114783b Pl 13 12 43.7855575272 -02 15 54.130663296           ~ 41 1
19 HD 114783 PM* 13 12 43.7855575272 -02 15 54.130663296 9.137 8.469 7.550 7.053 6.627 K1V 193 1
20 * tau Boo Ro* 13 47 15.7381720026 +17 27 24.809555600 5.02 4.98 4.49 4.09 3.85 F7IV-V 988 1
21 HD 128311 BY* 14 36 00.5602765558 +09 44 47.454573266 9.232 8.441 7.446 6.895 6.425 K3V 311 1
22 HD 164427 PM* 18 04 42.5969086224 -59 12 34.469434044   7.50 6.89     G0+V 62 1
23 HD 168443c Pl 18 20 03.9332862096 -09 35 44.614653900           ~ 93 1
24 HD 169822 SB* 18 26 10.0827771331 +08 46 39.150880145   8.52   7.4   G6V 112 0
25 HD 179949 BY* 19 15 33.2300695008 -24 10 45.671448072   6.772 6.237     F8V 405 1
26 HD 184860b Pl? 19 36 45.63937 -10 26 36.3596           ~ 4 1
27 HD 184860 ** 19 36 45.63937 -10 26 36.3596   9.41 8.40     K2+K7 55 1
28 HD 187123 PM* 19 46 58.1122487784 +34 25 10.281404460       7.4   G2V 246 1
29 HD 209458 V* 22 03 10.7727465312 +18 53 03.549393384   8.21 7.63     F9V 1115 1
30 * 51 Peg PM* 22 57 27.9804852576 +20 46 07.797040104 6.39 6.16 5.46 4.97 4.61 G2IV 1159 1
31 HD 217107 ** 22 58 15.5408995872 -02 23 43.383234768   6.919 6.163     G8IV/V 368 1

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