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A JUPITER-MASS COMPANION TO A SOLAR-TYPE STAR
Author(s): MAYOR M, QUELOZ D
Source: NATURE    Volume: 378    Issue: 6555    Pages: 355-359    Published: NOV 23 1995  
Times Cited: 1,214     References: 25     
Abstract: The presence of a Jupiter-mass companion to the star 51 Pegasi is inferred from observations of periodic variations in the star's radial velocity. The companion lies only about eight million kilometres from the star, which would be well inside the orbit of Mercury in our Solar System. This object might be a gas-giant planet that has migrated to this location through orbital evolution, or from the radiative stripping of a brown dwarf.
Document Type: Article
Language: English
Reprint Address: MAYOR, M (reprint author), OBSERV GENEVA, 51 CHEMIN MAILLETTES, CH-1290 SAUVERNY, SWITZERLAND
Publisher: MACMILLAN MAGAZINES LTD, 4 LITTLE ESSEX STREET, LONDON, ENGLAND WC2R 3LF
Subject Category: Multidisciplinary Sciences
IDS Number: TF893
ISSN: 0028-0836
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