Detailed Information on Publication Record
2021
Magnetic chemically peculiar stars investigated by the Solar Mass Ejection Imager
PAUNZEN, Ernst, Johana SUPÍKOVÁ, Klaus BERNHARD, Stefan HÜMMERICH, Michal PRIŠEGEN et. al.Basic information
Original name
Magnetic chemically peculiar stars investigated by the Solar Mass Ejection Imager
Authors
PAUNZEN, Ernst (40 Austria, guarantor, belonging to the institution), Johana SUPÍKOVÁ (203 Czech Republic, belonging to the institution), Klaus BERNHARD, Stefan HÜMMERICH and Michal PRIŠEGEN (703 Slovakia, belonging to the institution)
Edition
Monthly Notices of the Royal Astronomical Society, Oxford University Press, 2021, 0035-8711
Other information
Language
English
Type of outcome
Článek v odborném periodiku
Field of Study
10308 Astronomy
Country of publisher
United Kingdom of Great Britain and Northern Ireland
Confidentiality degree
není předmětem státního či obchodního tajemství
References:
Impact factor
Impact factor: 5.235
RIV identification code
RIV/00216224:14310/21:00121824
Organization unit
Faculty of Science
UT WoS
000656139300042
Keywords in English
stars: chemically peculiar; stars: early-type; Hertzsprung-Russell and colour-magnitude diagrams; stars: variables: general
Tags
Tags
International impact, Reviewed
Změněno: 24/6/2021 10:04, Mgr. Marie Šípková, DiS.
Abstract
V originále
Since the discovery of the spectral peculiarities of their prototype α2 Canum Venaticorum in 1897, the so-called ACV variables, which are comprised of several groups of chemically peculiar stars of the upper main sequence, have been the target of numerous photometric and spectroscopic studies. Especially for the brighter ACV variables, continuous observations over about a century are available, which are important to study long-term effects such as period changes or magnetic cycles in these objects. This work presents an analysis of 165 Ap/CP2 and He-weak/CP4 stars using light curves obtained by the Solar Mass Ejection Imager (SMEI) between the years 2003 and 2011. These data fill an important gap in observations for bright ACV variables between the Hipparcos and TESS satellite missions. Using specifically tailored data treatment and period search approaches, we find variability in the accuracy limit of the employed data in 84 objects. The derived periods are in excellent agreement with the literature; for one star, the here presented solution represents the first published period. We discuss the apparently constant stars and the corresponding level of non-variability. From an investigation of our target star sample in the Hertzsprung–Russell diagram, we deduce ages between 100 Myr and 1 Gyr for the majority of our sample stars. Our results support that the variable CP2/4 stars are in a more advanced evolutionary state and that He and Si peculiarities, preferentially found in the hotter, and thus more massive, CP stars, produce larger spots or spots of higher contrast.
Links
98507, interní kód MU |
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