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3 questions with no upvoted or accepted answers
3 votes
0 answers
48 views

Strength of core-envelope coupling in stars (again)

I asked this on the physics SE but it received little attention: Consider a high-mass zero-age main-sequence (ZAMS) (e.g., $m_{\rm ZAMS} \gtrsim 30\,$M$_{\odot}$) star. I understand that the core-...
Daddy Kropotkin's user avatar
2 votes
0 answers
90 views

The mass of Subdwarf B progenitors in the main sequence

Note: By "progenitor", I mean "the star as it was when it was still main sequence". Please correct me if I've got the terminology wrong. Most B-type subdwarfs have mass roughly half that of the Sun. ...
Astrid_Redfern's user avatar
1 vote
0 answers
63 views

Are there simplified M-L, M-R, and lifetime equations for non main sequence stars?

To give some context - I am trying to create a simple program that outputs the stellar properties of a star when given its initial mass and current age. e.g. Input Initial Mass = 2e30kg Age = 4.6 ...
Danni111111's user avatar