The Influence of X-ray Emission on the Stellar Wind of O Stars

Simple item page
dc.creatorKrticka, Jiri
dc.creatorKubat, Jiri
dc.date2006-07-26
dc.date.accessioned2026-07-07T07:15:47Z
dc.date.available2026-07-07T07:15:47Z
dc.descriptionWe study the influence of X-ray radiation on the wind parameters of O stars. For this purpose we use our own NLTE wind code. The X-ray emission (assumed to be generated in wind shocks) is treated as an input quantity. We study its influence on the mass-loss rate, terminal velocity and ionization state of the stellar wind of Galactic O stars.
dc.description2 pages; to appear in the proceedings of workshop "Mass loss from stars and the evolution of stellar clusters", A. de Koter, L. Smith & R. Waters, eds
dc.identifierhttps://arxiv.org/abs/astro-ph/0607595
dc.identifierhttp://arxiv.org/abs/astro-ph/0607595
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/113341
dc.subjectAstrophysics
dc.titleThe Influence of X-ray Emission on the Stellar Wind of O Stars
dc.typetext

Files

Collections

arXiv