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...
Main Authors: | , , |
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Format: | Article |
Language: | English |
Published: |
Odessa I. I. Mechnykov National University
2017-03-01
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Series: | Odessa Astronomical Publications |
Online Access: | http://oap.onu.edu.ua/article/view/93113 |