ANALYSIS OF THE SPECTRAL ENERGY DISTRIBUTION OFTHE COOLEST RCrB TYPE CARBON STAR DY Per

We analysed the spectral energy distribution of the evolved carbon star DY Per by spectral synthesis technique. The red giant shows the photometric features of R CrB type stars. We derived the atmosphere parameters of DY Per using three variants of molecular line lists. The range of Teff estimations...

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Bibliographic Details
Main Authors: L. A. Yakovina, A. V. Shavrina, Ya. V. Pavlenko, A. F. Pugach
Format: Article
Language:English
Published: Odessa I. I. Mechnykov National University 2008-12-01
Series:Odessa Astronomical Publications
Online Access:http://oap.onu.edu.ua/article/view/86884

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