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A binary merger origin for inflated hot Jupiter planets

Author
MARTIN, E. L1 ; SPRUIT, H. C2 ; TATA, R3
[1] Centro de Astrobiologia CSIC - INTA, Carretera Torrejón-Ajalvir km 4, 28850 Madrid, Spain
[2] Max-Planck-Institut fur Astrophysik, 85748 Garching, Germany
[3] Instituto de Astrofisica de Canarias, calle Via Lactea, 38200 La Laguna, Tenerife, Spain
Source

Astronomy and astrophysics (Berlin. Print). 2011, Vol 535 ; A50.1-A50.6 ; 1 ; ref : 3/4 p

CODEN
AAEJAF
ISSN
0004-6361
Scientific domain
Astronomy earth cosmic environment
Publisher
EDP Sciences, Les Ulis
Publication country
France
Document type
Article
Language
English
Author keyword
binaries: eclipsing blue stragglers methods: statistical planets and satellites: dynamical evolution and stability planets and satellites: formation
Keyword (fr)
Abondance Binaire détachée Binaire éclipse Blue straggler Cosmogonie planétaire Durée vie Etoile faible masse Etoile type T Tauri Evolution dynamique Inflation Masse stellaire Méthode statistique Orbite Paramètre physique Planète Jupiter Stabilité dynamique
Keyword (en)
Abundance Detached binary Eclipsing binary stars Blue stragglers Planetary cosmogony Lifetime Low-mass stars T Tauri stars Dynamical evolution Inflation Stellar mass Statistical method Orbits Physical parameter Jupiter planet Dynamic stability
Keyword (es)
Binario staccato Cosmogonía planetaria Evolución dinámica Método estadístico Parámetro físico
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
25505913

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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