The Open UniversitySkip to content

Ultraviolet studies of interacting binaries

Gaansicke, Boris T.; de Martino, Domitilla; Marsh, Thomas R.; Haswell, Carole A.; Knigge, Christian; Long, Knox S. and Shore, Steven N. (2006). Ultraviolet studies of interacting binaries. Astrophysics and Space Science, 303(1-4) pp. 53–68.

DOI (Digital Object Identifier) Link:
Google Scholar: Look up in Google Scholar


Interacting Binaries consist of a variety of stellar objects in different stages of evolution and those containing accreting compact objects still represent a major challenge to our understanding of not only close binary evolution but also of the chemical evolution of the Galaxy. These end-points of binary star evolution are ideal laboratories for the study of accretion and outflow processes, and provide insight on matter under extreme physical conditions. One of the key-questions of fundamental relevance is the nature of SN Ia progenitors. The study of accreting compact binary systems relies on observations over the entire electromagnetic spectrum and we outline here those unresolved questions for which access to the ultraviolet range is vital, as they cannot be addressed by observations in any other spectral region.

Item Type: Journal Article
ISSN: 1572-946X
Keywords: Close binaries; Cataclysmic variables; Symbiotic stars; X-ray binaries; Evolution; Accretion discs · Winds · Magnetism
Academic Unit/Department: Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
Interdisciplinary Research Centre: Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)
Item ID: 10904
Depositing User: Astrid Peterkin
Date Deposited: 25 Jun 2008
Last Modified: 04 Oct 2016 10:10
Share this page:


Scopus Citations

▼ Automated document suggestions from open access sources

Actions (login may be required)

Policies | Disclaimer

© The Open University   + 44 (0)870 333 4340