Model atmosphere of HD101065 with individualized abundances.

Abstract

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.

Keywords

• peculiar star
• model atmosphere
• individualized abundances
• hd101065