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Model atmosphere of HD101065 with individualized abundances.
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 p...
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Autori principali: | , |
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Natura: | Artigo |
Lingua: | Inglês |
Pubblicazione: |
Odessa I. I. Mechnykov National University
2017-03-01
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Serie: | Odessa Astronomical Publications |
Soggetti: | |
Accesso online: | http://oap.onu.edu.ua/article/view/95038 |
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