On the chemical abundances of stars with giant planets

• Tipo: Artigo em Livro de Atas de Conferência Internacional
• Data: 2006

Autores

N.C. Santos (Autor) Outra

Ata de Conferência Internacional

Título: Chemical Abundances and Mixing in Stars in the Milky Way and Its Satellites

Páginas: 19-22

ESO-Arcetri Workshop on Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites

Castiglione della Pescaia, ITALY, SEP 13-17, 2004

Indexação

ISI Web of Knowledge - 1 Citação

Scopus - 0 Citações

Outras Informações

ID Authenticus: P-004-PAE

DOI: 10.1007/978-3-540-34136-9_5

Abstract (EN): One particular fact that is helping us to understand the mechanisms of planetary formation has to do with the planet host stars themselves. In fact, these were found to have, on average, a metal content higher than the one found in stars without detected planetary companions. In this contribution we will mainly focus on the most recent results on the chemical abundances of planet-host stars, and what kind of constraints they are bringing to the theories of planet formation.

Idioma: Inglês

Tipo (Avaliação Docente): Científica

Nº de páginas: 4