On the semimajor axis distribution of extrasolar gas giant planets: Why hot Jupiters are rare around high-mass stars

Astrophysical Journal

Volumn 694, Issue 2 PART 2, 2009, Pages

  Currie, Thayne ^a  

^a HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

Author keywords

Formation; Planetary systems

Indexed keywords

EID: 66649136464     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/694/2/L171     Document Type: Article

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