IUE-spectra of the four interacting binary white dwarf stars: AM CVn, PG 1346+082, V803 Cen, AND GP com. A comparative study

Abstract This project is part of a world wide cooperation aimed at investigating properties of white dwarf stars to determine their constitution and evolution. The project is based on two recent developments: -The first is the discovery, of pulsational instabilities in some white dwarf stars, giving...
Ausführliche Beschreibung

Gespeichert in:

Autor*in:	Ulla, A. M. [verfasserIn] Solheim, J. -E.

Format:	Artikel
Sprache:	Englisch

Erschienen:	1990

Schlagwörter:	Mass Transfer Processed Material White Dwarf Dwarf Star Flux Modulation

Anmerkung:	© Kluwer Academic Publishers 1990

Übergeordnetes Werk:	Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 169(1990), 1-2 vom: Juli, Seite 189-192
Übergeordnetes Werk:	volume:169 ; year:1990 ; number:1-2 ; month:07 ; pages:189-192

Links:	Volltext

DOI / URN:	10.1007/BF00640709

Katalog-ID:	OLC2066180572

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title_auth	IUE-spectra of the four interacting binary white dwarf stars: AM CVn, PG 1346+082, V803 Cen, AND GP com. A comparative study
abstract	Abstract This project is part of a world wide cooperation aimed at investigating properties of white dwarf stars to determine their constitution and evolution. The project is based on two recent developments: -The first is the discovery, of pulsational instabilities in some white dwarf stars, giving rise to non-radial pulsations which can be observed as flux modulations with low amplitude. -The second is to study the mass transfer between interacting binary white dwarf stars, which transports processed material from the interior of the donating star to the accretor. We present a study of four interacting binary white dwarf systems based on IUE spectra. © Kluwer Academic Publishers 1990
abstractGer	Abstract This project is part of a world wide cooperation aimed at investigating properties of white dwarf stars to determine their constitution and evolution. The project is based on two recent developments: -The first is the discovery, of pulsational instabilities in some white dwarf stars, giving rise to non-radial pulsations which can be observed as flux modulations with low amplitude. -The second is to study the mass transfer between interacting binary white dwarf stars, which transports processed material from the interior of the donating star to the accretor. We present a study of four interacting binary white dwarf systems based on IUE spectra. © Kluwer Academic Publishers 1990
abstract_unstemmed	Abstract This project is part of a world wide cooperation aimed at investigating properties of white dwarf stars to determine their constitution and evolution. The project is based on two recent developments: -The first is the discovery, of pulsational instabilities in some white dwarf stars, giving rise to non-radial pulsations which can be observed as flux modulations with low amplitude. -The second is to study the mass transfer between interacting binary white dwarf stars, which transports processed material from the interior of the donating star to the accretor. We present a study of four interacting binary white dwarf systems based on IUE spectra. © Kluwer Academic Publishers 1990
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title_short	IUE-spectra of the four interacting binary white dwarf stars: AM CVn, PG 1346+082, V803 Cen, AND GP com. A comparative study
url	https://doi.org/10.1007/BF00640709
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author2	Solheim, J. -E.
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doi_str	10.1007/BF00640709
up_date	2024-07-04T03:55:56.194Z
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