A new synthetic model for asymptotic giant branch stars
R. G. IzzardInstitute of Astronomy, Madingley Road., Cambridge CB3 0HAChristopher A. ToutInstitute of Astronomy, Madingley Road., Cambridge CB3 0HAAmanda I. KarakasSchool of Mathematical Sciences, Monash University, Wellington Road, Clayton, Victoria 3800, AustraliaOnno R. PolsAstronomical Institute Utrecht, Postbus 80000, 3508 TA Utrecht, the Netherlands
2004en
ABI
Аннотация
We present a synthetic model for thermally pulsing asymptotic giant branch (TPAGB) evolution constructed by fitting expressions to full evolutionary models in the metallicity range 0.0001 ≤ Z ≤ 0.02. Our model includes parametrizations of third dredge
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Идентификаторлар
Иқтибослар ва манбалар
2 та иқтибос0 та фойдаланилган манба