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- Not counting the occasional [[supernova]], the first variable star to be identified was Mira or ''ο Ceti'' which was found to be periodically ...ry astronomer [[Friedrich Argelander]]. According to this system the first variable star discovered in any given constellation is designated ''R'' followed by the g18 KB (2,830 words) - 10:19, 9 June 2008
- 97 bytes (11 words) - 12:07, 2 June 2008
- *[http://www.aavso.org/ ''American Association of Variable Star Observers] .../www.sai.msu.su/groups/cluster/gcvs/gcvs/iii/vartype.txt Classification of variable star types]279 bytes (41 words) - 12:18, 2 June 2008
- Auto-populated based on [[Special:WhatLinksHere/Variable star]]. Needs checking by a human.466 bytes (60 words) - 21:27, 11 January 2010
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- *[http://www.aavso.org/ ''American Association of Variable Star Observers] .../www.sai.msu.su/groups/cluster/gcvs/gcvs/iii/vartype.txt Classification of variable star types]279 bytes (41 words) - 12:18, 2 June 2008
- {{rpl|Variable star}}178 bytes (21 words) - 03:19, 15 January 2010
- Variable star in the class of cataclysmic variable stars, which is normally very faint bu275 bytes (40 words) - 10:37, 28 October 2011
- {{r|Variable star}}393 bytes (49 words) - 10:31, 23 November 2011
- <noinclude>{{Subpages}}</noinclude>Pulsating variable star which exhibits a relation between period of variation and absolute luminosi203 bytes (29 words) - 13:49, 16 October 2008
- {{r|Variable star}} {{r|Cataclysmic variable star}}982 bytes (156 words) - 06:05, 19 July 2010
- ...n Association of VAriable Star Observers|AAVSO]] - American Association of VAriable Star Observers820 bytes (99 words) - 10:46, 19 October 2008
- The main component of ''α Andromedae'' is classified as a [[variable star]] of the α<sup>2</sup> Canum venaticorum variety. Its brightness varies be2 KB (285 words) - 17:19, 29 May 2008
- Wolf 359 is a variable star <ref>catalogued as variable star CN Leonis</ref> and flares periodically, growing dramatically in brightness3 KB (526 words) - 18:43, 20 December 2007
- Auto-populated based on [[Special:WhatLinksHere/Variable star]]. Needs checking by a human.466 bytes (60 words) - 21:27, 11 January 2010
- {{r|Variable star}}2 KB (213 words) - 09:18, 6 March 2024
- Like many globular clusters, NGC 7089 contains a number of [[variable star]]s, most notable of the ''RR Lyrae'' type. There are also 3 ''W Virginis''3 KB (450 words) - 11:11, 19 June 2008
- {{r|Variable star}}2 KB (310 words) - 21:24, 11 January 2010
- Proxima Centauri is a very active variable star. As a star of low mass it converts hydrogen to helium very slowly compared5 KB (794 words) - 18:54, 20 December 2007
- A '''supernova''' (plural ''supernovae''), is an exploding [[variable star]] object, that reaches a maximum brightness at about the magnitude of an en4 KB (664 words) - 16:43, 28 November 2010
- {{r|Variable star}}2 KB (323 words) - 12:57, 15 March 2024
- * R Leporis is an irregular variable star which was first described by the British astronomer [[John Russell Hind]] i1 KB (160 words) - 18:12, 30 December 2008
- Not counting the occasional [[supernova]], the first variable star to be identified was Mira or ''ο Ceti'' which was found to be periodically ...ry astronomer [[Friedrich Argelander]]. According to this system the first variable star discovered in any given constellation is designated ''R'' followed by the g18 KB (2,830 words) - 10:19, 9 June 2008
- *''[[Variable Star]]'' (posthumously with [[Spider Robinson]]) (Outline written by Heinlein 114 KB (1,905 words) - 05:23, 3 October 2013
- ...llar class]] G2 V, and about 4.6 Gyr in age. The sun is not considered a [[variable star]], but it does undergo periodic changes in activity known as the [[sunspot ...{{cite web | url = http://www.aavso.org/ | title = American Association of Variable Star Observers | publisher = AAVSO | language = English | accessdate = 2006-08-246 KB (6,796 words) - 10:08, 28 February 2024