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Rayleigh scattering in the atmospheres of hot stars

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F16%3A00090083" target="_blank" >RIV/00216224:14310/16:00090083 - isvavai.cz</a>

  • Alternative codes found

    RIV/67985815:_____/16:00463103

  • Result on the web

    <a href="http://dx.doi.org/10.1051/0004-6361/201628291" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201628291</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/0004-6361/201628291" target="_blank" >10.1051/0004-6361/201628291</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Rayleigh scattering in the atmospheres of hot stars

  • Original language description

    Context. Rayleigh scattering is a result of an interaction of photons with bound electrons. Rayleigh scattering is mostly neglected in calculations of hot star model atmospheres because most of the hydrogen atoms are ionized and the heavier elements have a lower abundance than hydrogen. In atmospheres of some chemically peculiar stars, helium overabundant regions containing singly ionized helium are present and Rayleigh scattering can be a significant opacity source. Aims. We evaluate the contribution of Rayleigh scattering by neutral hydrogen and singly ionized helium in the atmospheres of hot stars with solar composition and in the atmospheres of helium overabundant stars. Methods. We computed several series of model atmospheres using the TLUSTY code and emergent fluxes using the SYNSPEC code. These models describe atmospheres of main sequence B-type stars with different helium abundance.

  • 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/GA14-02385S" target="_blank" >GA14-02385S: Transfer of polarized radiation in stellar atmospheres</a><br>

  • Continuities

    S - Specificky vyzkum na vysokych skolach

Others

  • Publication year

    2016

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Astronomy & Astrophysics

  • ISSN

    1432-0746

  • e-ISSN

  • Volume of the periodical

    590

  • Issue of the periodical within the volume

    June

  • Country of publishing house

    FR - FRANCE

  • Number of pages

    6

  • Pages from-to

    "nestrankovano"

  • UT code for WoS article

    000378106800118

  • EID of the result in the Scopus database