Paczynski yıldız modellemesinde kullanılmak için opaklık tabloları ve onların yıldız evrimlerine etkileri

Yıldız modellemede Paczyski ’nin ücretsiz programı GOB’a uygulanabilir bir formatta kullanmak için opaklık tabloları oluşturduk. Tablolarımız, Lagrange interpolasyon yöntemi kullanılarak düşük metal içerikli zarflar için Allard ve Weiss ’in tablolarından elde edilmiştir. Bu, verilen hidrojen (X ), helyum (Y) ve metallerin (Z) oranları ile yoğunluk ve sıcaklığın sayısal bir fonksiyonu olarak doğru opaklıkların elde edilmesini sağlar. Inlek ve grubu opaklık etkilerini yüksek kalitede modern gözlemsel verilerden kontrol etmenin bağımsız olarak mümkün olduğunu göstermiştir. Bu tablolar bu tarz amaçlar için yararlı olacaktır.

Opacity tables for using in Paczynski stellar modelling and their effects on stellar evolutions

We have constructed opacity tables for using in stellar modelling in a format particularly applicable to the Paczynski freeware program GOB. Our tables are derived from those of Allard and Weiss for lower metal content envelopes, using the Lagrange interpolation method. This allows accurate opacities to be given as numerical functions of density and temperature with given proportions of hydrogen (X), helium (Y), and ‘metals’ (Z). Inlek et al. showed that it is possible independently to check opacity effects from modern high-quality observational data. These tables will be useful for such purposes.

Keywords:

Stars, general-structure opacity tables,

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