White Dwarfs in Post-Common Envelope Binaries

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F10%3A00373410" target="_blank" >RIV/67985815:_____/10:00373410 - 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 Dwarfs in Post-Common Envelope Binaries

Original language description

We examine the population of white dwarfs in post-common envelope binaries with a particular emphasis on the youngest objects and their ultraviolet properties. We present some results of our analysis of far ultraviolet spectroscopy of hot white dwarfs and the techniques employed to constrain their temperature, surface gravity and chemical composition. The results will be employed to improve distance estimates toward these objects and to calculate their space density. The measured abundance patterns alsoshow the effect of accretion of mass loss material from the secondary onto the white dwarf atmosphere.

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

5

Pages from-to

183-187

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

000289880000047