Low-Mass Companions for Five Solar-Type Stars From the Magellan Planet Search Program

We report low-mass companions orbiting five solar-type stars that have emerged from the Magellan precision Doppler velocity survey, with minimum (Msin i) masses ranging from 1.2 to 25 M JUP. These nearby target stars range from mildly metal-poor to metal-rich, and appear to have low chromospheric ac...

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Veröffentlicht in:The Astrophysical journal 2009-03, Vol.693 (2), p.1424-1430
Hauptverfasser: Minniti, Dante, Butler, R. Paul, López-Morales, Mercedes, Shectman, Stephen A, Adams, Fred C, Arriagada, Pamela, Boss, Alan P, Chambers, John E
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Sprache:eng
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Zusammenfassung:We report low-mass companions orbiting five solar-type stars that have emerged from the Magellan precision Doppler velocity survey, with minimum (Msin i) masses ranging from 1.2 to 25 M JUP. These nearby target stars range from mildly metal-poor to metal-rich, and appear to have low chromospheric activity. The companions to the brightest two of these stars have previously been reported from the CORALIE survey. Four of these companions (HD 48265-b, HD 143361-b, HD 28185-b, and HD 111232-b) are low-mass Jupiter-like planets in eccentric intermediate- and long-period orbits. On the other hand, the companion to HD 43848 appears to be a long-period brown dwarf in a very eccentric orbit.
ISSN:0004-637X
1538-4357
DOI:10.1088/0004-637X/693/2/1424