Ten low-mass companions from the Keck precision velocity survey
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作者:
Vogt, SS
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Univ Calif Santa Cruz, Univ Calif Observ, Lick Observ, Santa Cruz, CA 95064 USAUniv Calif Santa Cruz, Univ Calif Observ, Lick Observ, Santa Cruz, CA 95064 USA
Vogt, SS
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Butler, RP
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机构:Univ Calif Santa Cruz, Univ Calif Observ, Lick Observ, Santa Cruz, CA 95064 USA
Butler, RP
Marcy, GW
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机构:Univ Calif Santa Cruz, Univ Calif Observ, Lick Observ, Santa Cruz, CA 95064 USA
Marcy, GW
Fischer, DA
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机构:Univ Calif Santa Cruz, Univ Calif Observ, Lick Observ, Santa Cruz, CA 95064 USA
Fischer, DA
Pourbaix, D
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机构:Univ Calif Santa Cruz, Univ Calif Observ, Lick Observ, Santa Cruz, CA 95064 USA
Pourbaix, D
Apps, K
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机构:Univ Calif Santa Cruz, Univ Calif Observ, Lick Observ, Santa Cruz, CA 95064 USA
Apps, K
Laughlin, G
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Laughlin, G
机构:
[1] Univ Calif Santa Cruz, Univ Calif Observ, Lick Observ, Santa Cruz, CA 95064 USA
[2] Carnegie Inst Washington, Dept Terr Magnetism, Washington, DC 20015 USA
[3] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA
[4] San Francisco State Univ, Dept Phys & Astron, San Francisco, CA 94132 USA
Ten new companions have emerged from the Keck precision Doppler velocity survey, with minimum (M sin i) masses ranging from 0.8 M-JUP to 0.34 M.. Five of these are planet candidates with M sin i < 12 M-JUP, two are brown dwarf candidates with M sin i ∼ 30 M-JUP, 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 M-JUP toward the lowest detectable masses near 1 M-SAT.