NLTE models of Vela X-1 primary wind

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F10%3A00049701" target="_blank" >RIV/00216224:14310/10:00049701 - isvavai.cz</a>

Alternative codes found

RIV/67985815:_____/10:00373821

Result on the web

—

DOI - Digital Object Identifier

—

Result language

angličtina

Original language name

NLTE models of Vela X-1 primary wind

Original language description

We calculate NLTE models of the stellar wind of Vela X-1 primary. The predicted wind mass-loss rate and terminal velocity show good agreement with observations. The wind in the vicinity of the neutron star is strongly affected by X-ray photoionization. In accordance with observations, the wind velocity close to the neutron star is lower due to the presence of X-rays.

Czech name

—

Czech description

—

Type

D - Article in proceedings

CEP classification

BN - Astronomy and celestial mechanics, astrophysics

OECD FORD branch

—

Project

<a href="/en/project/GA205%2F07%2F0031" target="_blank" >GA205/07/0031: Stellar winds of first stars in the Universe</a><br>

Continuities

P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Publication year

2010

Confidentiality

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

Article name in the collection

BINARIES ? KEY TO COMPREHENSION OF THE UNIVERSE

ISBN

978-1-58381-750-6

ISSN

—

e-ISSN

—

Number of pages

2

Pages from-to

405-406

Publisher name

Astronomical Society of the Pacific

Place of publication

San Francisco, USA

Event location

Brno

Event date

Jan 1, 2009

Type of event by nationality

WRD - Celosvětová akce

UT code for WoS article

000289880000102