A&A 430, 1143-1154 (2005)
DOI: 10.1051/0004-6361:20034563
A catalog of stellar magnetic rotational phase curves
V. D. Bychkov1, 2, L. V. Bychkova1 and J. Madej31 Special Astrophysical Observatory of the Russian Academy of Sciences, Nizhnij Arkhyz, 369167 Russia
e-mail: vbych@sao.ru
2 Isaac Newton Institute of Chile, SAO Branch, Nizhnij Arkhyz, 369167 Russia
3 Astronomical Observatory, University of Warsaw, Al. Ujazdowskie 4, 00-478 Warszawa, Poland
(Received 22 October 2003 / Accepted 20 September 2004)
Abstract
Magnetized stars usually exhibit periodic variations of the effective
(longitudinal) magnetic field
caused by their rotation. We present a
catalog of magnetic rotational phase curves,
vs. the rotational
phase
, and tables of their parameters
for 136 stars on
the main sequence and above it.
Phase curves were obtained
by the least squares fitting of sine wave or double wave functions to the
available
measurements, which were compiled from the existing literature.
Most of the catalogued objects are chemically
peculiar A and B type stars (127 stars). For some stars we also improved or
determined periods of their rotation. We discuss the distribution of
parameters describing magnetic rotational phase curves in our sample.
Key words: catalogs -- stars: fundamental parameters -- stars: magnetic fields -- stars: rotation
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© ESO 2005
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