Confirmation of the planet hypothesis for the long-period radial velocity variations of β Geminorum

Astronomy and Astrophysics

Volumn 457, Issue 1, 2006, Pages 335-341

  Hatzes, A P ^a   Cochran, W D ^b   Endl, M ^b   Guenther, E W ^a   Saar, S H ^c   Walker, G A H ^d   Yang, S ^e   Hartmann, M ^a   Esposito, M ^a   Paulson, D B ^f   Dollinger M P ^g  

^a THÜRINGER LANDESSTERNWARTE TAUTENBURG   (Germany)

^b The University of Texas at Austin   (United States)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^d University of Victoria ^*  (Canada)

^e UNIVERSITY OF VICTORIA   (Canada)

^f NASA GODDARD SPACE FLIGHT CENTER   (United States)

^g EUROPEAN SOUTHERN OBSERVATORY   (Germany)

Author keywords

Planetary systems; Star: individual: Gem; Techniques: radial velocities

Indexed keywords

ASTRONOMY; ASTROPHYSICS; OPTICAL RESOLVING POWER; PHOTOMETRY; SPECTRUM ANALYSIS;

PLANET-FORMATION; PLANETARY SYSTEMS; STAR: INDIVIDUAL: ΒGEM; TECHNIQUES: RADIAL VELOCITIES;

VELOCITY MEASUREMENT;

EID: 33749049571     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20065445     Document Type: Article

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