Three regimes of extrasolar planet radius inferred from host star metallicities.

Buchhave, Lars A; Bizzarro, Martin; Latham, David W; Sasselov, Dimitar; Cochran, William D; Endl, Michael; Isaacson, Howard; Juncher, Diana; Marcy, Geoffrey W

Buchhave, Lars A; Bizzarro, Martin; Latham, David W; Sasselov, Dimitar; Cochran, William D; Endl, Michael; Isaacson, Howard; Juncher, Diana; Marcy, Geoffrey W.

Afiliación

Buchhave LA; 1] Harvard-Smithsonian Center for Astrophysics, Cambridge, Massachusetts 02138, USA [2] Centre for Star and Planet Formation, Natural History Museum of Denmark, University of Copenhagen, DK-1350 Copenhagen, Denmark.
Bizzarro M; Centre for Star and Planet Formation, Natural History Museum of Denmark, University of Copenhagen, DK-1350 Copenhagen, Denmark.
Latham DW; Harvard-Smithsonian Center for Astrophysics, Cambridge, Massachusetts 02138, USA.
Sasselov D; Harvard-Smithsonian Center for Astrophysics, Cambridge, Massachusetts 02138, USA.
Cochran WD; McDonald Observatory, The University of Texas, Austin, Texas 78712, USA.
Endl M; McDonald Observatory, The University of Texas, Austin, Texas 78712, USA.
Isaacson H; University of California, Berkeley, California 94720, USA.
Juncher D; 1] Centre for Star and Planet Formation, Natural History Museum of Denmark, University of Copenhagen, DK-1350 Copenhagen, Denmark [2] Niels Bohr Institute, University of Copenhagen, DK-2100 Copenhagen, Denmark.
Marcy GW; University of California, Berkeley, California 94720, USA.

Nature ; 509(7502): 593-5, 2014 May 29.

Article en En | MEDLINE | ID: mdl-24870544

Texto completo

Imprimir

XML

PubMed Links

Buscar en Google

Texto completo: 1 Colección: 01-internacional Banco de datos: MEDLINE Idioma: En Revista: Nature Año: 2014 Tipo del documento: Article País de afiliación: Dinamarca

Texto completo

Imprimir

XML

PubMed Links

Buscar en Google