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- W2997516244 abstract "Massive stars lose a considerable amount of mass during their lifetime. When the star explodes as a supernova (SN), the resulting shock wave expands in the medium created by the stellar mass-loss. Thermal X-ray emission from the SN depends on the square of the density of the ambient medium, which in turn depends on the mass-loss rate (and velocity) of the progenitor wind. The emission can therefore be used to probe the stellar mass-loss in the decades or centuries before the star's death. We have aggregated together data available in the literature, or analysed by us, to compute the X-ray lightcurves of almost all young supernovae detectable in X-rays. We use this database to explore the mass-loss rates of massive stars that collapse to form supernovae. Mass-loss rates are lowest for the common Type IIP supernovae, but increase by several orders of magnitude for the highest luminosity X-ray SNe." @default.
- W2997516244 created "2020-01-10" @default.
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- W2997516244 date "2018-08-01" @default.
- W2997516244 modified "2023-09-27" @default.
- W2997516244 title "Massive star mass-loss revealed by X-ray observations of young supernovae" @default.
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- W2997516244 doi "https://doi.org/10.1017/s1743921318008438" @default.
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