For those interested on the Luminous Blue Variables, check out this paper: [[1]]. I suggest to check the HTML version; it includes several tables with "bona-fid
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| On 2 February 2013, it was proposed that this article be moved to Luminous blue variable. The result of the discussion was moved. |
For those interested on the Luminous Blue Variables, check out this paper: [[1]]. I suggest to check the HTML version; it includes several tables with "bona-fide" LBVs as well as candidates.
The theoretical Mass Limit mentioned in Hypergiants is 120, while here it says 150. It does vary slightly depending on the star's composition, but isn't this too high? --Acoyauh (talk) 00:26, 18 January 2008 (UTC)
"Hypergiants should not be confused with luminous blue variables. A hypergiant is classified as such because of its size and mass loss rate, whereas a luminous blue variable is thought to be a massive blue supergiant going through an evolutionary phase where it loses a large amount of mass." - page on Hypergiants. "Luminous blue variables...are very bright, blue, hypergiant variable stars" - LBV I don't have any expertise in the area to correct it, but this seems a blatant contradiction that would be worth bringing up. 72.187.145.13 (talk) 22:39, 4 April 2009 (UTC)
I think that the term hypernova is used improperly. Saying "If they were any larger, their gravity would be insufficient to balance their radiation pressure and they would blow themselves apart in a hypernova" implies that super Eddington luminosity is the direct cause of a hypernova. This is not the case. A hypernova marks the death of the most massive stars following the collapse of the core into a black hole. This doesn't have anything to do with a large luminosity blowing off the stars outer layers. —Preceding unsigned comment added by 128.118.147.106 (talk) 19:55, 9 June 2009 (UTC)
Deleted. —Preceding unsigned comment added by 91.182.140.200 (talk) 12:10, 11 October 2009 (UTC)
The article states that the luminous blue variable is "named after S Doradus, the brightest star of the Large Magellanic Cloud." This statement contradicts with this article http://en.wikipedia.org/wiki/Most_luminous_stars where it's apparent that R136a1, part of the same Large Magellanic Cloud, is the most luminous star at this moment.
There is a list in the article of what are described as "some of the best known" LBVs. Most of them are not especially well known at all, but the list is far from a complete list of all LBVs. There is also a Wikipedia category for LBVs which is even shorter than the list in this article. This should really be rationalised and certainly the category needs to be at least as complete as any list we make in this article. The list of galactic stars confirmed as LBVs is really very short at about a dozen and could easily go in the article. Then there are a handful more in other local group galaxies. The list of candidate LBVs, stars very likely to be LBVs but not studied long enough or in enough detail to be positive, is perhaps a bit too long and most are meaningless numbers from IR and X-Ray surveys, but a few certainly deserve mention. — Preceding unsigned comment added by Lithopsian (talk • contribs) 13:41, 8 July 2012 (UTC)
The result of the proposal was moved. --BDD (talk) 19:03, 11 February 2013 (UTC) (non-admin closure)
Luminous blue variable star → Luminous blue variable – In nearly all fields, these stars are known as luminous blue variables (LBVs) and are not specifically called luminous blue variable stars, since that is tacitly implied (as all LBVs are stars). Therefore, WP:COMMONNAME applies, and this article should be moved. StringTheory11 (t • c) 04:05, 2 February 2013 (UTC)
*'''Support''' or *'''Oppose''', then sign your comment with ~~~~. Since polling is not a substitute for discussion, please explain your reasons, taking into account Wikipedia's policy on article titles.It has been suggested that this section be split out into another page titled List of luminous blue variables. (Discuss) |
I think that the list is rather long, so should be split off into a separate list article -- 65.92.180.137 (talk) 07:13, 28 February 2013 (UTC)
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