Modeling rapidly rotating stars

Simple item page
dc.creatorRieutord, M.
dc.date2007-02-14
dc.date.accessioned2026-07-07T07:46:45Z
dc.date.available2026-07-07T07:46:45Z
dc.descriptionWe review the quest of modeling rapidly rotating stars during the past 40 years and detail the challenges to be taken up by models facing new data from interferometry, seismology, spectroscopy... We then present the progress of the ESTER project aimed at giving a physically self-consistent model for the structure and evolution of rapidly rotating stars.
dc.descriptionto appear in the proceedings of the SF2A conference held in Paris June 2006. 6p. 1 fig
dc.identifierhttps://arxiv.org/abs/astro-ph/0702384
dc.identifierhttp://arxiv.org/abs/astro-ph/0702384
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/123933
dc.subjectAstrophysics
dc.titleModeling rapidly rotating stars
dc.typetext

Files

Collections

arXiv