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”

Stability analysis of radial oscillation modes in massive stars

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F24%3A00616785" target="_blank" >RIV/67985815:_____/24:00616785 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1017/S1743921322003143" target="_blank" >http://dx.doi.org/10.1017/S1743921322003143</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1017/S1743921322003143" target="_blank" >10.1017/S1743921322003143</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Stability analysis of radial oscillation modes in massive stars

  • Original language description

    During the evolution of massive stars, their properties change significantly. But stellar parameters of massive stars have the biggest uncertainties in stellar astrophysics, specifically in the post-main sequence stages where blue supergiant stars are located. These stars experience mass loss events during their evolution which are supposed to be related to strange-modes instabilities. In this work, we explore the stability of oscillation modes in massive stars for different masses, and a range of mass-loss rates, with the aim to provide clues about the connection between strange modes instabilities and mass-loss events.n

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    <a href="/en/project/GA20-00150S" target="_blank" >GA20-00150S: Structure and evolution of stellar ejecta</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

  • Article name in the collection

    Proceedings of the International Astronomical Union

  • ISBN

  • ISSN

    1743-9213

  • e-ISSN

    1743-9221

  • Number of pages

    2

  • Pages from-to

    251-252

  • Publisher name

    Cambridge University Press

  • Place of publication

    Cambridge

  • Event location

    Ballyconnell

  • Event date

    May 8, 2022

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article