Evolutionary models for cool brown dwarfs and extrasolar giant planets. The case of HD 209458

Astronomy and Astrophysics

Volumn 402, Issue 2, 2003, Pages 701-712

  Baraffe, I ^a,b   Chabrier, G ^a   Barman, T S ^c   Allard, F ^a   Hauschildt, P H ^d  

^a CENTRE DE RECHERCHE ASTROPHYSIQUE DE LYON   (France)

^b MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^c WICHITA STATE UNIVERSITY   (United States)

^d UNIVERSITY OF HAMBURG   (Germany)

Author keywords

Planetary systems; Stars: brown dwarfs; Stars: evolution; Stars: individual (HD 209458)

Indexed keywords

INFRARED RADIATION; IRRADIATION; MATHEMATICAL MODELS; PLANETS; SOLAR ENERGY;

PLANETRY SYSTEMS;

ASTROPHYSICS;

EID: 0038680604     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20030252     Document Type: Article

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