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Effect of rotational mixing and metallicity on the hot star wind mass-loss rates

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F14%3A00073775" target="_blank" >RIV/00216224:14310/14:00073775 - isvavai.cz</a>

  • Alternative codes found

    RIV/67985815:_____/14:00433746

  • Result on the web

    <a href="http://dx.doi.org/10.1051/0004-6361/201423845" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201423845</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/0004-6361/201423845" target="_blank" >10.1051/0004-6361/201423845</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Effect of rotational mixing and metallicity on the hot star wind mass-loss rates

  • Original language description

    Hot star wind mass-loss rates depend on the abundance of individual elements. This dependence is usually accounted for assuming scaled solar chemical composition. However, this approach may not be justified in evolved rotating stars. The rotational mixing brings CNO-processed material to the stellar surface, increasing the abundance of nitrogen at the expense of carbon and oxygen, which potentially influences the mass-loss rates. We study the influence of the modified chemical composition resulting fromthe rotational mixing on the wind parameters, particularly the wind mass-loss rates. We use our NLTE wind code to predict the wind structure and compare the calculated wind mass-loss rate for the case of scaled solar chemical composition and the composition affected by the CNO cycle. We show that for a higher mass-fraction of heavier elements Z/Zo&gt;0.

  • 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/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)

Others

  • Publication year

    2014

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Astronomy and Astrophysics

  • ISSN

    0004-6361

  • e-ISSN

  • Volume of the periodical

    567

  • Issue of the periodical within the volume

    JULY

  • Country of publishing house

    FR - FRANCE

  • Number of pages

    7

  • Pages from-to

    "A63-1"-"A63-7"

  • UT code for WoS article

    000341185300123

  • EID of the result in the Scopus database