Display title | Astronomy:Dwarf nova |
Default sort key | Dwarf nova |
Page length (in bytes) | 7,319 |
Namespace ID | 3024 |
Namespace | Astronomy |
Page ID | 467776 |
Page content language | en - English |
Page content model | wikitext |
Indexing by robots | Allowed |
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Page image |  |
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Page creator | imported>WikiG |
Date of page creation | 06:48, 6 February 2024 |
Latest editor | imported>WikiG |
Date of latest edit | 06:48, 6 February 2024 |
Total number of edits | 1 |
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Description | Content |
Article description: (description ) This attribute controls the content of the description and og:description elements. | A dwarf nova (pl. novae), or U Geminorum variable, is one of several types of cataclysmic variable star, consisting of a close binary star system in which one of the components is a white dwarf that accretes matter from its companion. Dwarf novae are dimmer and repeat more frequently than "classical... |