Exploring the brown dwarf desert : new substellar companions from the SDSS-III MARVELS survey

Planet searches using the radial velocity technique show a paucity of companions to solar-type stars within ∼5 au in the mass range of ∼10–80 MJup. This deficit, known as the brown dwarf desert, currently has no conclusive explanation. New substellar companions in this region help assess the reality...

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Detalhes bibliográficos
Autores: Grieves, Nolan, Ge, Jian, Thomas, N., Ma, Bo, Sithajan, Sirinrat, Ghezzi, Luan, Kimock, Benjamin, Willis, Kevin, De Lee, Nathan M., Lee, Brian L., Fleming, S.W., Agol, Eric, Troup, Nicholas W., Paegert, Martin, Schneider, D.P., Stassun, Keivan G., Városi, Frank, Zhao, Bo, Liu, Jian, Li, Rui, Mello, Gustavo Frederico Porto de, Bizyaev, D., Pan, K., Ferreira, Letícia D., Lorenzo-Oliveira, Diego, Santiago, Basilio Xavier, Costa, Luiz N. da, Maia, Marcio Antonio Geimba, Ogando, Ricardo L.C., Del Peloso, Eduardo Fernandez
Formato: artículo
Estado:Versión publicada
Fecha de publicación:2017
País:Brasil
Recursos:Universidade Federal do Rio Grande do Sul (UFRGS)
Repositorio:Repositório Institucional da UFRGS
Idioma:inglés
OAI Identifier:oai:www.lume.ufrgs.br:10183/159732
Acesso em linha:http://hdl.handle.net/10183/159732
Access Level:acceso abierto
Palavra-chave:Anãs marrons
Velocidade radial
Estrelas binarias
Techniques radial velocities
Binaries spectroscopic
Brown dwarfs
Descrição
Resumo:Planet searches using the radial velocity technique show a paucity of companions to solar-type stars within ∼5 au in the mass range of ∼10–80 MJup. This deficit, known as the brown dwarf desert, currently has no conclusive explanation. New substellar companions in this region help assess the reality of the desert and provide insight to the formation and evolution of these objects. Here, we present 10 new brown dwarf and 2 low-mass stellar companion candidates around solar-type stars from the Multi-object APO Radial Velocity Exoplanet Large-Area Survey (MARVELS) of the Sloan Digital Sky Survey III. These companions were selected from processed MARVELS data using the latest University of Florida Two Dimensional pipeline, which shows significant improvement and reduction of systematic errors over previous pipelines. The 10 brown dwarf companions range in mass from ∼13 to 76 MJup and have orbital radii of less than 1 au. The two stellar companions have minimum masses of ∼98 and 100 MJup. The host stars of the MARVELS brown dwarf sample have a mean metallicity of [Fe/H] = 0.03 ± 0.08 dex. Given our stellar sample we estimate the brown dwarf occurrence rate around solar-type stars with periods less than ∼300 d to be ∼0.56 per cent.

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