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          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents



ID: 710192.0, MPI für Astronomie / Publikationen_mpia
Physical parameters of young M-type stars and brown dwarfs with VOSA
Authors:Bayo, A.; Rodrigo, C.; Barrado, D.; Solano, E.; Allard, F.; Joergens, V.
Date of Publication (YYYY-MM-DD):2014-01
Audience:Not Specified
Abstract / Description:Although M dwarfs are the most common stars in our stellar neighborhood they are still among the least understood. This class of objects is dominated by dramatic changes: in their interiors (fully convective, with implications in angular momentum evolution), in their atmospheres (crossing temperatures where dust settling occurs), and in their nature (including both, stellar and substellar objects). Populating efficiently our solar neighborhood, they are very well represented in the databases coming from new and more sensitive surveys that provide photometry at many wavelength ranges and cover large areas of the sky (few examples among many others are GALEX, SDSS, 2MASS, WISE and VISTA). In this context of opulence of objects and data, the Virtual Observatory comes in naturally as an excellent framework to efficiently advance in the knowledge of M-type sources. We put special emphasis in the benefits of using the new capabilities of VOSA (Virtual Observatory SED Analyzer, (2008A&A...492..277B); in operation since 2008 and in constant development) to study large samples of candidate and confirmed M members of Chamaeleon I.
Free Keywords:stars: low-mass; brown dwarfs; stars: fundamental parameters; infrared: stars; stars: formation
External Publication Status:published
Document Type:Other
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:URL:http://adsabs.harvard.edu/abs/2014ASInC..11...93B
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