White Dwarf Companions to Luminous Stars

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F10%3A00373402" target="_blank" >RIV/67985815:_____/10:00373402 - isvavai.cz</a>

Result on the web

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DOI - Digital Object Identifier

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Result language

angličtina

Original language name

White Dwarf Companions to Luminous Stars

Original language description

We derive properties of white dwarf companions to luminous stars by means of ultraviolet spectroscopy. The Lyman line profiles constrain the temperature and gravity of the white dwarfs. The parameters are used to estimate the white dwarf ages and massesenabling a study of the binary birth and evolution and possible constraints on the initial mass ratios.

Czech name

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Czech description

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Type

D - Article in proceedings

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

P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>Z - Vyzkumny zamer (s odkazem do CEZ)

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

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e-ISSN

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Number of pages

2

Pages from-to

189-190

Publisher name

Astronomical Society of the Pacific

Place of publication

San Francisco

Event location

Brno

Event date

Jun 8, 2009

Type of event by nationality

WRD - Celosvětová akce

UT code for WoS article

000289880000048