About: Mass fluxes for O-type supergiants with metallicity Z = Z⊙/5

Documentation

scienceplus.abes.fr version Bêta

scienceplus.abes.fr | explorer

À propos de : Mass fluxes for O-type supergiants with metallicity Z = Z⊙/5 Goto Sponge NotDistinct Permalink

Attributs	Valeurs
type	work Article
Is Part Of	http://hub.abes.fr/edp/periodical/aa/2015/volume_582/issue_2015/w
Subject	stars: mass-loss stars: winds, outflows Stellar atmospheres stars: early-type
Title	Mass fluxes for O-type supergiants with metallicity Z = Z⊙/5
Date	2015-01-01(xsd:dateTime)
has manifestation of work	http://hub.abes.fr/edp/periodical/aa/2015/volume_582/issue_2015/aa26882-15/m/print http://hub.abes.fr/edp/periodical/aa/2015/volume_582/issue_2015/aa26882-15/m/web
related by	http://hub.abes.fr/edp/periodical/aa/2015/volume_582/issue_2015/aa26882-15/authorship/1
Author	Lucy, L. B.
Abstract	A code used previously to predict O-star mass fluxes as a function of metallicity is used to compute a grid of models with the metallicity of the Small Magellanic Cloud (SMC). These models allow mass-loss rates to be derived by interpolation for all O-type supergiants in the SMC, with the possible exception of extremely massive stars close to the Eddington limit.
article type	research-article
publisher identifier	aa26882-15
Date Copyrighted	2015-01-01(xsd:dateTime)
Rights	© ESO, 2015
Rights Holder	ESO
is part of this journal	Astronomy & Astrophysics
is primary topic of	http://hub.abes.fr/edp/periodical/aa/2015/volume_582/issue_2015/aa26882-15/w/record

Alternative Linked Data Documents: ODE Content Formats:

RDF

ODATA

Microdata