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Publikováno v:
Monthly Notices of the Royal Astronomical Society. 475:4881-4890
A linear stability analysis of models for evolved primordial stars with masses between 150 and 250 M$_{\odot}$ is presented. Strange mode instabilities with growth rates in the dynamical range are identified for stellar models with effective temperat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a478d74283a745d5d446be94520d23a1
https://doi.org/10.1093/mnras/sty092
https://doi.org/10.1093/mnras/sty092
