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RAS PhysicsАстрономический журнал Astronomy Reports

  • ISSN (Print) 0004-6299
  • ISSN (Online) 3034-5170

SPECTROSCOPIC BINARY CEPHEID AU PEG IN GAIA DR3 EPOCH: THE ELLIPSOIDALITY EFFECT, MASS AND EVOLUTIONARY STATUS

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PII
S30345170S0004629925040061-1
DOI
10.7868/S3034517025040061
Publication type
Article
Status
Published
Authors
A. S. Rastorguev
  • Affiliation:
    Lomonosov Moscow State University, Faculty of Physics
    Lomonosov Moscow State University, Sternberg Astronomcal Institute
M. V. Zabolotskikh
  • Affiliation: Lomonosov Moscow State University, Sternberg Astronomcal Institute
N. A. Gorynya
  • Affiliation:
    Lomonosov Moscow State University, Sternberg Astronomcal Institute
    Institute of Astronomy of the RAS
Volume/ Edition
Volume 102 / Issue number 4
Pages
317-330
Abstract
The physical parameters and evolutionary status of the spectroscopic binary Cepheid AU Peg, usually classified as a BL Her variable, are revised. Taking into account previously unpublished radial velocity measurements made with the correlation spectrometer, the parameters of the relative orbit of the system are refined. Based on 74 new radial velocity measurements made in the period
Keywords
двойные и кратные звезды AU Peg звездная эволюция фундаментальные параметры звезд
Date of publication
25.12.2024
Year of publication
2024
Number of purchasers
0
Views
38

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