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...
Egile Nagusiak: | Han, Z, Podsiadlowski, P, Maxted, P, Marsh, T, Ivanova, N |
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Formatua: | Conference item |
Argitaratua: |
2002
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Antzeko izenburuak
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The origin of subdwarf B stars - I. The formation channels
nork: Han, Z, et al.
Argitaratua: (2002) -
The origin of subdwarf B star - I: The formation channels
nork: Han, Z, et al.
Argitaratua: (2002) -
The origin of subdwarf B stars - II
nork: Han, Z, et al.
Argitaratua: (2003) -
Subdwarf B stars from the common envelope ejection channel
nork: Xiong, H, et al.
Argitaratua: (2017) -
Editorial: special issue on hot subdwarf stars
nork: Han, Z, et al.
Argitaratua: (2010)