MODELS OF ENERGY DISTRIBUTION IN SPECTRUM OF SAKURAFS OBJECT

Theoretical energy distributions in a spectrum of Sakurai's object (SO) are calculated for a grid of hydrogen-deficient and carbon-rich model atmospheres of Teff = 5000-6200 K and log g= 0.0-1.0. Model atmospheres of SO are computed by the technique of opacity sampling with account of atomic an...

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Bibliographic Details
Main Authors: Ya. Pavlenko, L. Yakovina, H. W. Duerbeck
Format: Article
Language:English
Published: Odessa I. I. Mechnykov National University 2017-03-01
Series:Odessa Astronomical Publications
Online Access:http://oap.onu.edu.ua/article/view/93113

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