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Y CVn (La Superbathis) is too faint to call a red supergiant. The luminosity of Y CVn is 4,400 times solar. Meanwhile that of Mira is 8,400 times solar. Y CVn is less luminous than Mira. Mira is a M7III type normal red giant. Therefore , Y CVn should be a normal red giant.
The classification "I" in the spectral type "C7I" of Y CVn means "Most luminous class of carbon stars". But this class is too faint to call red supergaint's class.
Reference information : List of M type giant stars.
1 Most luminous supergiant(hypergiant)
2 Luminous supergiant(Ia type).
3 Faint supergiants(Ib type).
4 Bright giant(II type).
5 Normal giant(III type).
Kometsuga 14:12, 9 March 2007 (UTC)
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![]() | This article is rated Start-class on Wikipedia's
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Y CVn (La Superbathis) is too faint to call a red supergiant. The luminosity of Y CVn is 4,400 times solar. Meanwhile that of Mira is 8,400 times solar. Y CVn is less luminous than Mira. Mira is a M7III type normal red giant. Therefore , Y CVn should be a normal red giant.
The classification "I" in the spectral type "C7I" of Y CVn means "Most luminous class of carbon stars". But this class is too faint to call red supergaint's class.
Reference information : List of M type giant stars.
1 Most luminous supergiant(hypergiant)
2 Luminous supergiant(Ia type).
3 Faint supergiants(Ib type).
4 Bright giant(II type).
5 Normal giant(III type).
Kometsuga 14:12, 9 March 2007 (UTC)
Hello fellow Wikipedians,
I have just modified one external link on La Superba. Please take a moment to review my edit. If you have any questions, or need the bot to ignore the links, or the page altogether, please visit this simple FaQ for additional information. I made the following changes:
When you have finished reviewing my changes, you may follow the instructions on the template below to fix any issues with the URLs.
This message was posted before February 2018.
After February 2018, "External links modified" talk page sections are no longer generated or monitored by InternetArchiveBot. No special action is required regarding these talk page notices, other than
regular verification using the archive tool instructions below. Editors
have permission to delete these "External links modified" talk page sections if they want to de-clutter talk pages, but see the
RfC before doing mass systematic removals. This message is updated dynamically through the template {{
source check}}
(last update: 5 June 2024).
Cheers.— InternetArchiveBot ( Report bug) 00:25, 15 December 2017 (UTC)