Talk:SCR 1845−6357: Difference between revisions

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Red or brown dwarf?

This page and List of nearest stars both list SCR 1845-6357 A as a red dwarf. However, both the Nasa link at the bottom of List of nearest stars and Template:Nearest systems say that SCR 1845-6357 A is a late-M class brown dwarf. Which one is it? Adeptzare3 (talk) 04:27, 1 December 2013 (UTC)[reply]

Mass measurements for component A are still approximate, so it could be either. All we can really be sure of at the moment is that it's somewhere in the vicinity of the hydrogen-burning limit.--203.57.211.237 (talk) 07:35, 23 April 2016 (UTC)[reply]

Discoverer constellation designation

Using a discoverer constellation designation SCR 1845-6357 would be Biller Pavonis or Biller Pav. Astredita (talk) 12:57, 19 May 2014 (UTC)[reply]

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 ==Red or brown dwarf?==
 This page and [[List of nearest stars]] both list SCR 1845-6357 A as a red dwarf. However, both the Nasa link at the bottom of [[List of nearest stars]] and [[Template:Nearest systems]] say that SCR 1845-6357 A is a late-M class brown dwarf. Which one is it? [[User:Adeptzare3|Adeptzare3]] ([[User talk:Adeptzare3|talk]]) 04:27, 1 December 2013 (UTC)
+:Mass measurements for component A are still approximate, so it could be either. All we can really be sure of at the moment is that it's somewhere in the vicinity of the hydrogen-burning limit.--[[Special:Contributions/203.57.211.237|203.57.211.237]] ([[User talk:203.57.211.237|talk]]) 07:35, 23 April 2016 (UTC)
 == Discoverer constellation designation ==