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pro vyhledávání: '"Harita Palani Balaji"'
Publikováno v:
The Astrophysical Journal. 933:194
Red supergiant stars lose a lot of mass in slow winds that forms a circumstellar medium (CSM) around the star. When the star retains a substantial hydrogen envelope at the time of explosion, it displays characteristic light curves and spectra of a Ty
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::df1592442350c7ef1780d35e3bb69ef9
https://doi.org/10.3847/1538-4357/ac7528
https://doi.org/10.3847/1538-4357/ac7528
