All

What are you looking for?

All
Projects
Results
Organizations

Quick search

  • Projects supported by TA ČR
  • Excellent projects
  • Projects with the highest public support
  • Current projects

Smart search

  • That is how I find a specific +word
  • That is how I leave the -word out of the results
  • “That is how I can find the whole phrase”

Hot subdwarf wind models with accurate abundances: II. Helium-dominated merger products CD-46 8926 and CD-51 11879

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F24%3A00585242" target="_blank" >RIV/67985815:_____/24:00585242 - isvavai.cz</a>

  • Alternative codes found

    RIV/00216224:14310/24:00135876

  • Result on the web

    <a href="https://hdl.handle.net/11104/0353272" target="_blank" >https://hdl.handle.net/11104/0353272</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/0004-6361/202347978" target="_blank" >10.1051/0004-6361/202347978</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Hot subdwarf wind models with accurate abundances: II. Helium-dominated merger products CD-46 8926 and CD-51 11879

  • Original language description

    We aim to understand the influence of modified surface abundances on the strength of the stellar wind in the helium-dominated subdwarfs CD-46 8926 and CD-51 11879. A modified wind strength could resolve the problem with the X-ray emission of these stars, as the expected X-ray luminosity of both stars is significantly higher than the upper limit determined from observations. We used our own optical spectroscopy combined with archival ultraviolet spectroscopy and photometry to derive basic parameters and surface abundances of selected subdwarfs. The resulting parameterst served as input for the METUJE stellar wind code, which predicts the wind structure of these stars. We compared the derived wind parameters with the predictions derived for solar abundances.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    <a href="/en/project/GA22-34467S" target="_blank" >GA22-34467S: Binary interaction on the red giant branch: Hot subdwarfs as a test case.</a><br>

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2024

  • 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

    0004-6361

  • e-ISSN

    1432-0746

  • Volume of the periodical

    683

  • Issue of the periodical within the volume

    March

  • Country of publishing house

    FR - FRANCE

  • Number of pages

    10

  • Pages from-to

    A80

  • UT code for WoS article

    001181364400009

  • EID of the result in the Scopus database

    2-s2.0-85187234163