The Boundaries of the GW Vir Stars in the Effective Temperature - Surface Gravity Domain

Simple item page
dc.creatorQuirion, P. -O.
dc.creatorFontaine, G.
dc.creatorBrassard, P.
dc.date2006-10-14
dc.date.accessioned2026-07-07T07:26:58Z
dc.date.available2026-07-07T07:26:58Z
dc.descriptionWe derive the theoretical red edge of the pulsating GW Vir stars by using full evolutionary calculations that involve mass loss and diffusion. We put the emphasis on the fact that the specific mass loss law used in the evolutionary computations determines the red edge's position. By combining this specific property with the observed location of the red edge in the effective temperature-surface gravity domain, we obtain interesting constraints on possible mass loss laws for PG 1159 stars.
dc.description6 pages 2 figures, 15th European Workshop on White Dwarfs
dc.identifierhttps://arxiv.org/abs/astro-ph/0610443
dc.identifierhttp://arxiv.org/abs/astro-ph/0610443
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/117218
dc.subjectAstrophysics
dc.titleThe Boundaries of the GW Vir Stars in the Effective Temperature - Surface Gravity Domain
dc.typetext

Files

Collections

arXiv