The formation of subdwarf B stars
We performed full binary evolution calculations and carried out binary population synthesis studies in order to investigate the formation of subdwarf B (sdB) stars via, the channels of stable Roche lobe overflow (RLOF), common envelope ejection and helium white dwarf mergers. Our model is successful...
Príomhchruthaitheoirí: | Han, Z, Podsiadlowski, P, Maxted, P, Marsh, T, Ivanova, N |
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Formáid: | Conference item |
Foilsithe / Cruthaithe: |
2002
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Míreanna comhchosúla
Míreanna comhchosúla
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