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  • Photometrically and spectroscopically variable chemically peculiar (CP) stars are the optimum laboratories for testing the rotational evolution of main sequence stars. A vast majority of well-studied CP stars have quite steady rotational periods (e. g. SrCrEu star CQ UMa). However, there are several CP stars that exhibit apparent period variations. The origin of the period variations is unclear in many cases. We describe the observed period variations of several individual CP stars, especially V901 Ori, sigma Ori E, HR 7355, CU Vir, SX Ari, and EE Dra. The CP stars with unsteady periods now represent a very diverse group with dissimilar O-C diagrams and time scales. We also discuss the causes of the period changes found and a possible cyclicity or chaoticity of them.
  • Photometrically and spectroscopically variable chemically peculiar (CP) stars are the optimum laboratories for testing the rotational evolution of main sequence stars. A vast majority of well-studied CP stars have quite steady rotational periods (e. g. SrCrEu star CQ UMa). However, there are several CP stars that exhibit apparent period variations. The origin of the period variations is unclear in many cases. We describe the observed period variations of several individual CP stars, especially V901 Ori, sigma Ori E, HR 7355, CU Vir, SX Ari, and EE Dra. The CP stars with unsteady periods now represent a very diverse group with dissimilar O-C diagrams and time scales. We also discuss the causes of the period changes found and a possible cyclicity or chaoticity of them. (en)
Title
  • Magnetic Chemically Peculiar stars With Unsteady Periods
  • Magnetic Chemically Peculiar stars With Unsteady Periods (en)
skos:prefLabel
  • Magnetic Chemically Peculiar stars With Unsteady Periods
  • Magnetic Chemically Peculiar stars With Unsteady Periods (en)
skos:notation
  • RIV/00216224:14310/11:00049646!RIV12-GA0-14310___
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • P(GA205/06/0217), P(GA205/08/0003), S
http://linked.open...vai/riv/dodaniDat
http://linked.open...aciTvurceVysledku
http://linked.open.../riv/druhVysledku
http://linked.open...iv/duvernostUdaju
http://linked.open...titaPredkladatele
http://linked.open...dnocenehoVysledku
  • 210207
http://linked.open...ai/riv/idVysledku
  • RIV/00216224:14310/11:00049646
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • magnetic stars; CP stars; rotation (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...ontrolniKodProRIV
  • [AB6A3EFAA6CA]
http://linked.open...v/mistoKonaniAkce
  • Special Astrophysical Observatory of the Russian
http://linked.open...i/riv/mistoVydani
  • Moskva
http://linked.open...i/riv/nazevZdroje
  • Magnetic Stars. Proceedings of the International Conference, held in the Special Astrophysical Observatory of the Russian AS
http://linked.open...in/vavai/riv/obor
http://linked.open...ichTvurcuVysledku
http://linked.open...cetTvurcuVysledku
http://linked.open...vavai/riv/projekt
http://linked.open...UplatneniVysledku
http://linked.open...iv/tvurceVysledku
  • Janík, Jan
  • Mikulášek, Zdeněk
  • Zejda, Miloslav
  • Zvěřina, Pavel
  • Krtička, Jiří
  • Zverko, Juraj
  • Žižnovský, Jozef
http://linked.open...vavai/riv/typAkce
http://linked.open.../riv/zahajeniAkce
number of pages
http://purl.org/ne...btex#hasPublisher
  • Special Astrophysical Observatory of the Russian AS
https://schema.org/isbn
  • 978-5-7422-3156-1
http://localhost/t...ganizacniJednotka
  • 14310
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