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Magnetic Chemically Peculiar stars With Unsteady Periods

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F11%3A00049646" target="_blank" >RIV/00216224:14310/11:00049646 - isvavai.cz</a>

  • Result on the web

  • DOI - Digital Object Identifier

Alternative languages

  • Result language

    angličtina

  • Original language name

    Magnetic Chemically Peculiar stars With Unsteady Periods

  • Original language description

    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.

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

    BN - Astronomy and celestial mechanics, astrophysics

  • OECD FORD branch

Result continuities

  • Project

    Result was created during the realization of more than one project. More information in the Projects tab.

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>S - Specificky vyzkum na vysokych skolach

Others

  • Publication year

    2011

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Article name in the collection

    Magnetic Stars. Proceedings of the International Conference, held in the Special Astrophysical Observatory of the Russian AS

  • ISBN

    978-5-7422-3156-1

  • ISSN

  • e-ISSN

  • Number of pages

    9

  • Pages from-to

    52-60

  • Publisher name

    Special Astrophysical Observatory of the Russian AS

  • Place of publication

    Moskva

  • Event location

    Special Astrophysical Observatory of the Russian

  • Event date

    Aug 31, 2010

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article