dc.date.accessioned2019-12-18T18:14:37Z
dc.date.accessioned2022-10-18T22:33:25Z
dc.date.available2019-12-18T18:14:37Z
dc.date.available2022-10-18T22:33:25Z
dc.date.created2019-12-18T18:14:37Z
dc.date.issued2009
dc.identifierhttp://hdl.handle.net/10533/237039
dc.identifier15010003
dc.identifierWOS:000264095100033
dc.identifiereid=2-s2.0-69549123484
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4468377
dc.description.abstractWe report low mass companions orbiting five Solar-type stars that have emerged from the Magellan precision Doppler velocity survey, with minimum (Msini) masses ranging from 1.2 to 25 Mjup. 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, 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.
dc.languageeng
dc.relationhttps://arxiv.org/abs/0810.5348
dc.relation10.1088/0004-637X/693/2/1424
dc.relationinfo:eu-repo/grantAgreement/Fondap/15010003
dc.relationinstname: Conicyt
dc.relationreponame: Repositorio Digital RI2.0
dc.rightsinfo:eu-repo/semantics/openAccess
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.titleLow-Mass Companions for Five Solar-Type Stars From the Magellan Planet Search Program
dc.typeArticulo


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