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- W4295092372 abstract "According to recent analyses of the type-Ia supernova rate as a function of redshift, delayed and prompt type-Ia supernovae (SN Ia) should explode respectively in the Galactic bulge and in the nuclear bulge, a gas rich structure with ongoing star formation, located in the central region of the Milky Way. We estimate the rate of type-Ia supernovae in the Galactic bulge and nuclear bulge. We show that this rate is insufficient by an order of magnitude to explain by positron escape from type-Ia supernovae envelopes alone the large positron injection rate into the Galactic central region, as re-observed recently by the Spectrometer on INTEGRAL, which amounts to 1.25 10^{43} e+ s^{-1} and would require 0.5 SN Ia explosions per century." @default.
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- W4295092372 date "2006-09-20" @default.
- W4295092372 modified "2023-10-16" @default.
- W4295092372 title "Type Ia Supernova Rate in the Galactic Center Region" @default.
- W4295092372 doi "https://doi.org/10.48550/arxiv.astro-ph/0609566" @default.
- W4295092372 hasPublicationYear "2006" @default.
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