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Publikováno v:
The Astrophysical Journal. 617:1316-1322
Recent theoretical predictions for low metallicity massive stars predict that these stars should have drastically reduced equatorial winds (mass loss) while on the main sequence, and as such should retain most of their angular momentum. Observations
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a82d2be7d0594642ef03d2ad8f798a5c
https://doi.org/10.1086/425573
https://doi.org/10.1086/425573
