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Cataclysmic variables

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journal contribution
posted on 2023-06-07, 15:10 authored by Robert Connon Smith
Cataclysmic variables are binary stars in which a relatively normal star is transferring mass to its compact companion. This interaction gives rise to a rich range of behaviour, of which the most noticeable are the outbursts that give the class its name. Novae belong to the class, as do the less well known dwarf novae and magnetic systems. Novae draw their energy from nuclear reactions, while dwarf novae rely on gravity to power their smaller eruptions. All the different classes of cataclysmic variable can be accommodated within a single framework and this article will describe the framework, review the properties of the main types of system and discuss models of the outbursts and of the long-term evolution.

History

Publication status

  • Published

File Version

  • Accepted version

Journal

Contemporary Physics

ISSN

0010-7514

Publisher

Taylor & Francis

Issue

6

Volume

47

Page range

363-386

Department affiliated with

  • Physics and Astronomy Publications

Full text available

  • Yes

Peer reviewed?

  • Yes

Legacy Posted Date

2009-11-09

First Open Access (FOA) Date

2018-03-19

First Compliant Deposit (FCD) Date

2018-03-19

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