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Talk:Classical Cepheid variable

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This is an old revision of this page, as edited by Elphion (talk | contribs) at 01:09, 30 October 2015 (a good source?). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.
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Light curve characteristics

It would be nice to explain what sets Cepheids apart from other variable stars. I have read (in Modern Theories of the Universe from Herschel to Hubble) that what characterises a Cepheid is its light curve, with a relatively sharp and a slower decline. Can someone elaborate more? CielProfond (talk) 01:15, 15 December 2010 (UTC)[reply]

The obvious missing column in the table

... is the Luminosity. Distance and/or absolute magnitude would also be nice. With the table as it stands, the classic relationship that makes these stars important is not evident. -- Elphion (talk) 20:42, 29 October 2015 (UTC)[reply]

Great idea - want to add a column? If not I will do it sometime in the next few weeks. Cas Liber (talk · contribs) 00:30, 30 October 2015 (UTC)[reply]
I tried looking for the data, found what looked like conflicting stories. If you can point me to a good source I can try to do the honors. Otherwise happy to let you do the heavy lifting. -- Elphion (talk) 01:08, 30 October 2015 (UTC)[reply]