Talk:KW Sagittarii: Difference between revisions
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== {{solar radius|1,460}} == |
== {{solar radius|1,460}} == |
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Is the {{solar radius|1,460}} estimate even obsolete? I think it is. <span style="background-color: lime">'''[[User:Joey717|<span style="color:red">Joey717</span>]]'''</span> <sup>([[User talk:Joey717|talk]])</sup> 07:50, 9 September 2018 (UTC) |
Is the {{solar radius|1,460}} estimate even obsolete? I think it is. <span style="background-color: lime">'''[[User:Joey717|<span style="color:red">Joey717</span>]]'''</span> <sup>([[User talk:Joey717|talk]])</sup> 07:50, 9 September 2018 (UTC) |
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:It's certainly "older" than the other estimates, but I think it is still useful. Levesque et al. marked a significant step change in the temperature scale of cool supergiants, and for our purposes contained a self-consistent set of data for a large number of red supergiants. In this particular case it also forms an interesting comparison with the direct (assuming a distance) angular measurement of Arroyo-Torres. [[User:Lithopsian|Lithopsian]] ([[User talk:Lithopsian|talk]]) 10:32, 9 September 2018 (UTC) |
Latest revision as of 15:08, 30 January 2024
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1,460 R☉
[edit]Is the 1,460 R☉ estimate even obsolete? I think it is. Joey717 (talk) 07:50, 9 September 2018 (UTC)
- It's certainly "older" than the other estimates, but I think it is still useful. Levesque et al. marked a significant step change in the temperature scale of cool supergiants, and for our purposes contained a self-consistent set of data for a large number of red supergiants. In this particular case it also forms an interesting comparison with the direct (assuming a distance) angular measurement of Arroyo-Torres. Lithopsian (talk) 10:32, 9 September 2018 (UTC)