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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%2F15%3A00080776" target="_blank" >RIV/00216224:14310/15:00080776 - isvavai.cz</a>

  • Alternative codes found

    RIV/67985815:_____/15:00455428

  • Result on the web

  • DOI - Digital Object Identifier

Alternative languages

  • Result language

    angličtina

  • Original language name

    Rayleigh Scattering in the Atmospheres of Hot Stars

  • Original language description

    Rayleigh scattering is the process of interaction of photons with bound electrons. This process is often neglected in hot star model atmospheres. The reason is that a large fraction of hydrogen and helium atoms are singly ionized, and the scattering cross section of singly ionized helium is by two orders of magnitude lower than the neutral hydrogen scattering cross section. We studied the effect of Rayleigh scattering by neutral hydrogen and singly ionized helium in the stellar model atmospheres. We computed the models for the B-type stars with solar composition and helium overabundant atmospheres N(He)/N(H)=10. The results show that Rayleigh scattering by singly ionized helium can be a significant opacity source for the helium-rich stars, and this process can be included in hot star model atmospheres.

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

    BN - Astronomy and celestial mechanics, astrophysics

  • OECD FORD branch

Result continuities

  • Project

    <a href="/en/project/GA13-10589S" target="_blank" >GA13-10589S: Mass loss in hot massive stars</a><br>

  • Continuities

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

Others

  • Publication year

    2015

  • Confidentiality

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

Data specific for result type

  • Article name in the collection

    Physics and Evolution of Magnetic and Related Stars

  • ISBN

    9781583818732

  • ISSN

  • e-ISSN

  • Number of pages

    7

  • Pages from-to

    273-279

  • Publisher name

    Astronomical Society of the Pacific

  • Place of publication

    San Francisco

  • Event location

    Nizhny Arkhyz, Russia

  • Event date

    Aug 25, 2014

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article

    000366452300033