Atmospheric Models of Flare Stars: The Quiescent State of Ad Leo

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dc.creatorMauas, P.
dc.creatorFalchi, A.
dc.date1993-08-06
dc.date.accessioned2026-07-07T02:18:49Z
dc.date.available2026-07-07T02:18:49Z
dc.descriptionWe compute a semi-empirical atmospheric model for the dMe star AD Leo, which constitutes the first model computed to match the continuum observations, as well as a wide set of chromospheric spectral lines. We find good agreement between the computed and observed spectral features, with the exception of the Ca II K line.
dc.description13 pages, 10 figures available upon request, tex dialect, ARCETRI-PR-93-29
dc.identifierhttps://arxiv.org/abs/astro-ph/9308010
dc.identifierhttp://arxiv.org/abs/astro-ph/9308010
dc.identifierAstron.Astrophys. 281 (1994) 129-138
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9635
dc.subjectAstrophysics
dc.titleAtmospheric Models of Flare Stars: The Quiescent State of Ad Leo
dc.typetext

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