Model atmosphere of HD101065 with individualized abundances

Автор(и)

  • S. A. Khan Department of Astronomy, Tavrian National University after V.I. Vernadskiy, Ukraine
  • D. V. Shulyak Department of Astronomy, Tavrian National University after V.I. Vernadskiy, Ukraine

DOI:

https://doi.org/10.18524/1810-4215.2002.15.95038

Ключові слова:

peculiar star, model atmosphere, individualized abundances, HD101065

Анотація

We have calculated the model atmosphere of extremely peculiar roAp star HD101065. The line opacity with individualized abundances has been executed by "line-by-line" method. Due to lack of data for the REE lines we scaled D.R.E.A.M. data base by ten. The synthetic spectrum and indices in photometric system uvby have been calculated as: b-y = 0.713, m1 = 0.336, c1 = ?0.121. We had obtained good agreement between an observation and modelling.

Посилання

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Опубліковано

2017-03-07

Номер

Том 15 (2002)

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Відповідно Закону України про авторське право і суміжні права N 3792-XII від 23 грудня 1993 року