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The initial - Final mass relation for close low- and intermediate-mass binaries

Abstract:

Using Eggleton's stellar evolution code, we carry out 150 runs of Pop 1 binary evolution calculations with initial primary mass between 1 and 8M(circle dot), the initial mass ratio q = M-1/M-2 between 1.1 and 4, and the onset of Roche lobe overflow (RLOF) at an early, middle, or late phase in the Hertzsprung gap. We assume that the RLOF is conservative in the calculations and find that the remnant mass of the primary may change by more than 40 per cent over the range of initial mass ratio or ...

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Publication status:
Published

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Volume:
229
Pages:
217-221
Publication date:
2001-01-01
URN:
uuid:9482e5a5-6e7e-4604-b6d3-e26281f095d9
Source identifiers:
30023
Local pid:
pubs:30023
ISBN:
1-58381-061-7
Keywords:

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