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Study of Slowly Rotating CP Stars Observed with TESS

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F20%3A00118440" target="_blank" >RIV/00216224:14310/20:00118440 - isvavai.cz</a>

  • Result on the web

    <a href="https://www.pta.edu.pl/pliki/proc/vol11/v11p214.pdf" target="_blank" >https://www.pta.edu.pl/pliki/proc/vol11/v11p214.pdf</a>

  • DOI - Digital Object Identifier

Alternative languages

  • Result language

    angličtina

  • Original language name

    Study of Slowly Rotating CP Stars Observed with TESS

  • Original language description

    Since the end of 2018, the Transiting Exoplanet Survey Satellite (TESS) provides high-quality space data on stellar photometry to the astronomical community. We present the results of an analysis of TESS photometric data for known slowly rotating, magnetic, chemically peculiar (mCP) stars. In general, mCP stars show an inhomogeneous distribution of elements in their stellar atmospheres that leads to spectroscopic (line profile) and photometric (light curve) variations over the rotation period. In the frame of the oblique magnetic rotator (OMR) model, patches of enhanced chemical abundance on the stellar surface reveal the frequency of stellar rotation. Using this approach, we have compiled a list of slowly rotating mCP stars with rotation periods longer than two days from the analysis of the photometric data provided by TESS for the first eight sectors of observations. Slowly rotating mCP stars usually possess a hydrodynamically stable stellar atmosphere where a magnetic field can amplify the process of atomic diffusion and this leads to the horizontal and vertical stratification of chemical abundances.

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2020

  • Confidentiality

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

Data specific for result type

  • Article name in the collection

    Proceedings of the Polish Astronomical Society, Vol. 11

  • ISBN

    9788395043093

  • ISSN

    2545-1022

  • e-ISSN

  • Number of pages

    5

  • Pages from-to

    214-218

  • Publisher name

    Polskie Towarzystwo Astronomiczne

  • Place of publication

    Warszawa

  • Event location

    London (Canada)

  • Event date

    Jul 8, 2019

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article