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Rotational properties of magnetic chemically peculiar stars

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F18%3A00102567" target="_blank" >RIV/00216224:14310/18:00102567 - isvavai.cz</a>

  • Result on the web

    <a href="https://www.ta3.sk/caosp/Eedition/Abstracts/2018/Vol_48/No_1/pp194-202_abstract.html" target="_blank" >https://www.ta3.sk/caosp/Eedition/Abstracts/2018/Vol_48/No_1/pp194-202_abstract.html</a>

  • DOI - Digital Object Identifier

Alternative languages

  • Result language

    angličtina

  • Original language name

    Rotational properties of magnetic chemically peculiar stars

  • Original language description

    The magnetic chemically peculiar (mCP) stars of the upper main sequence exhibit strong and globally organized magnetic fields that are inclined to the rotational axis and facilitate the development of surface abundance inhomogeneities resulting in photometric and spectroscopic variability. Photometric time series data are much easier to obtain than spectroscopic/polarimetric data or are available from large surveys, thus the number of known rotational periods increased significantly during the last years. Furthermore, Gaia data allow us to place an unprecedentedly large sample of mCP stars in the Hertzsprung-Russell diagram and to investigate evolutionary effects. In this paper we review the rotational properties of mCP stars and discuss open issues of stellar rotation in the presence of strong magnetic fields.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

  • Continuities

    S - Specificky vyzkum na vysokych skolach<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2018

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Contributions of the Astronomical Observatory Skalnaté Pleso

  • ISSN

    1335-1842

  • e-ISSN

    1336-0337

  • Volume of the periodical

    48

  • Issue of the periodical within the volume

    1

  • Country of publishing house

    SK - SLOVAKIA

  • Number of pages

    9

  • Pages from-to

    194-202

  • UT code for WoS article

    000432791300027

  • EID of the result in the Scopus database

    2-s2.0-85042634958