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A search for photometric variability in magnetic chemically peculiar stars using ASAS-3 data

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F15%3A00085398" target="_blank" >RIV/00216224:14310/15:00085398 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1051/0004-6361/201526424" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201526424</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/0004-6361/201526424" target="_blank" >10.1051/0004-6361/201526424</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    A search for photometric variability in magnetic chemically peculiar stars using ASAS-3 data

  • Original language description

    The (magnetic) chemically peculiar (CP) stars of the upper main sequence are well-suited laboratories for investigating the influence of magnetic fields on the stellar surface because they produce abundance inhomogeneities (spots), which results in photometric variability that is explained in terms of the oblique rotator model. CP stars exhibiting this phenomenon are normally classified as alpha2 Canum Venaticorum (ACV) variables. It is important to increase the sample of known rotational periods amongCP stars by discovering new ACV variables. The ASAS-3 data were cross-correlated with the Catalogue of Ap, HgMn, and Am stars in order to analyse the light curves of bona fide CP and related stars. The light curves were downloaded and cleaned of outliersand data points with a flag indicating bad quality. Promising candidates showing a larger scatter than observed for constant stars in the corresponding magnitude range were searched for periodic signals using a standard Fourier technique

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

  • CEP classification

    BN - Astronomy and celestial mechanics, astrophysics

  • OECD FORD branch

Result continuities

  • Project

    <a href="/en/project/7AMB14AT015" target="_blank" >7AMB14AT015: Shed more light on magnetic stars</a><br>

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Others

  • Publication year

    2015

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    ASTRONOMY &amp; ASTROPHYSICS

  • ISSN

    1432-0746

  • e-ISSN

  • Volume of the periodical

    581

  • Issue of the periodical within the volume

    September

  • Country of publishing house

    FR - FRANCE

  • Number of pages

    32

  • Pages from-to

    "nestrankovano"

  • UT code for WoS article

    000361803900138

  • EID of the result in the Scopus database