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dc.contributor.authorBaraffe, I.
dc.contributor.authorChabrier, G.
dc.contributor.authorAllard, F.
dc.contributor.authorHauschildt, P.
dc.date.accessioned2015-04-15T12:50:08Z
dc.date.issued1998
dc.identifier.citationVol. 337, pp. 403 - 412en_GB
dc.identifier.urihttp://hdl.handle.net/10871/16831
dc.language.isoenen_GB
dc.publisherEDP Sciences for European Southern Observatory (ESO)en_GB
dc.relation.urlhttp://aa.springer.de/bibs/8337002/2300403/small.htmen_GB
dc.relation.urlhttp://arxiv.org/abs/astro-ph/9805009v1en_GB
dc.subjectstars: low-mass, brown dwarfsen_GB
dc.subjectstars: evolutionen_GB
dc.subjectstars: Hertzsprung-Russel (HR) and C-M diagramsen_GB
dc.subjectstars: interiorsen_GB
dc.subjectstars: atmospheresen_GB
dc.titleEvolutionary models for solar metallicity low-mass stars: mass-magnitude relationships and color-magnitude diagramsen_GB
dc.typeArticleen_GB
dc.date.available2015-04-15T12:50:08Z
dc.identifier.issn0004-6361
dc.descriptionCopyright © European Southern Observatory (ESO) 1998en_GB
dc.identifier.eissn1432-0746
dc.identifier.journalAstronomy and Astrophysicsen_GB


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