Talk:B-type main-sequence star

Tip: Anchors are case-sensitive in most browsers.

This article contains broken links to one or more target anchors:

[[Stellar classification#Type B|spectral type B]] The anchor (#Type B) is no longer available because it was deleted by a user before.

The anchors may have been removed, renamed, or are no longer valid. Please fix them by following the link above, checking the page history of the target pages, or updating the links.

Remove this template after the problem is fixed | Report an error

Bad move

To me it was a really, really bad idea to move this from "B-type main sequence star" to "B-type main sequence" because there is no such thing as a "B-type main sequence". The article name may now cause unnecessary confusion. It should have been discussed first. Regards, RJH (talk) 18:40, 21 March 2012 (UTC)[reply]

Move discussion in progress

There is a move discussion in progress on Talk:A-type main sequence star which affects this page. Please participate on that page and not in this talk page section. Thank you. —RMCD bot 22:44, 24 April 2013 (UTC)[reply]

luminosity needed

One of the most important properties of B-type main sequence stars is missing: what is their luminosity? "extremely luminous and blue" in the current version is vague. Bkocsis (talk) 11:42, 18 March 2020 (UTC)[reply]

Helium fusion

I would add that these stars transition to helium fusion more smoothly than solar mass stars, which experience a degenerate helium flash. 74.135.194.87 (talk) 16:57, 27 January 2024 (UTC)[reply]