Really focused stellar winds in X-ray binaries

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F12%3A00386677" target="_blank" >RIV/67985815:_____/12:00386677 - isvavai.cz</a>

Result on the web

<a href="http://dx.doi.org/10.1051/0004-6361/201016046" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201016046</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1051/0004-6361/201016046" target="_blank" >10.1051/0004-6361/201016046</a>

Result language

angličtina

Original language name

Really focused stellar winds in X-ray binaries

Original language description

We model numerically the stellar wind from a supergiant component of a binary in radial and three-dimensional radiation hydrodynamic approximation taking into account the Roche potential, Coriolis force, and radiative pressure in the continuum and spectral lines. The Coriolis force influences substantially the mass loss and thus also the accretion rate. The focusing of the stellar wind by the gravitational field of the compact companion leads to the formation of a gaseous tail behind the companion.

Czech name

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Czech description

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Type

J_x - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

CEP classification

BN - Astronomy and celestial mechanics, astrophysics

OECD FORD branch

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Project

Result was created during the realization of more than one project. More information in the Projects tab.

Continuities

Z - Vyzkumny zamer (s odkazem do CEZ)

Publication year

2012

Confidentiality

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Name of the periodical

Astronomy & Astrophysics

ISSN

0004-6361

e-ISSN

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Volume of the periodical

542

Issue of the periodical within the volume

June

Country of publishing house

FR - FRANCE

Number of pages

11

Pages from-to

"A42/1"-"A42/11"

UT code for WoS article

000305803300003

EID of the result in the Scopus database

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