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The Investigations of Variations in the Depression λ4200, λ5200 of the Magnetic Stars 53 Cam and Beta CrB

Published online by Cambridge University Press:  12 April 2016

V.I. Burnashev ,
V.P. Malanushenko  and
N.S. Polosukhina
V.I. Burnashev
Affiliation:
Crimean Astrophysical Observatory Crimea, Nauchny, 334413, U.S.S.R.
V.P. Malanushenko
Affiliation:
Crimean Astrophysical Observatory Crimea, Nauchny, 334413, U.S.S.R.
N.S. Polosukhina
Affiliation:
Crimean Astrophysical Observatory Crimea, Nauchny, 334413, U.S.S.R.

Extract

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During many recent years, from 1973, the search for short-term variations in the spectrum of Ap-stars has been carried out at the Crimean Astrophysical Observatory. Some results are presented in the poster dedicated to 53CAM observations. Spectral observations of the magnetic star 53CAM with time resolution of about I min were supplemented by the narrow-band photometrical observations within the framework of the cooperative program of the magnetic stars observations, started in 1979.

Type
Section III - Magnetic CP Stars
Information
International Astronomical Union Colloquium , Volume 90: Upper Main Sequence Stars with Anomalous Abundances , 1986 , pp. 341 - 344
Copyright
Copyright © Reidel 1986