The Nature of the Progenitors of Supernovae of Type-I

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

This paper examines the hypothesis that supernovae of type I are
produced by relatively "young" single stars. The fact that SN I are not
concentrated in spiral arms implies that their progenitors have M ⪉
8 M_sun;. The existence of white dwarfs in open clusters places a limit
M ⪆ 5 M_sun; on SN I progenitors.

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