Fundamental Parameters of CP Stars Observed at the 6-m Telescope. I. Observations in 2009–2011
- Authors: Moiseeva A.V.1, Romanyuk I.I.1, Semenko E.A.1, Kudryavtsev D.O.1, Yakunin I.A.1
-
Affiliations:
- Special Astrophysical Observatory
- Issue: Vol 74, No 1 (2019)
- Pages: 62-65
- Section: Article
- URL: https://journals.rcsi.science/1990-3413/article/view/212844
- DOI: https://doi.org/10.1134/S1990341319010061
- ID: 212844
Cite item
Abstract
The paper presents the results of determination of fundamental parameters (effective temperature, surface gravity, luminosity, mass, radius, rotation velocity, and radial velocity) for 146 stars observed at the 6-m telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences with the Main Stellar Spectrograph during 2009–2011; 124 of the stars are magnetic or potentially magnetic objects. We obtained and analyzed at least 500 pairs of circularly-polarized-emission spectra. Various methods and approaches were used in estimating the fundamental parameters.
About the authors
A. V. Moiseeva
Special Astrophysical Observatory
Author for correspondence.
Email: amoiseeva@sao.ru
Russian Federation, Nizhnii Arkhyz, 369167
I. I. Romanyuk
Special Astrophysical Observatory
Email: amoiseeva@sao.ru
Russian Federation, Nizhnii Arkhyz, 369167
E. A. Semenko
Special Astrophysical Observatory
Email: amoiseeva@sao.ru
Russian Federation, Nizhnii Arkhyz, 369167
D. O. Kudryavtsev
Special Astrophysical Observatory
Email: amoiseeva@sao.ru
Russian Federation, Nizhnii Arkhyz, 369167
I. A. Yakunin
Special Astrophysical Observatory
Email: amoiseeva@sao.ru
Russian Federation, Nizhnii Arkhyz, 369167
Supplementary files
