Shulyak D. Stellar model atmospheres of main sequence CP stars

Українська версія

Thesis for the degree of Candidate of Sciences (CSc)

State registration number

0406U001179

Applicant for

Specialization

  • 01.03.02 - Астрофізика, радіоастрономія

24-03-2006

Specialized Academic Board

К 41.051.04

Essay

This thesis describes the methodology of modeling of stellar model atmospheres of CP stars with stratified abundances and magnetic field. The stellar model atmosphere code is presented. The model atmospheres of CU Vir have been calculated with Si and Fe stratification. Model atmospheres have been computed taking into account Zeeman effect. The model atmospheres of Theta Aur with magnetic pressure effects are computed. The Stark effect parameters of some SiI and CrI lines are corrected. Field of use: astrophysics.

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