Dust grains from the heart of supernovae

Dust grains are classically thought to form in the winds of asymptotic giant branch (AGB) stars. However, there is increasing evidence today for dust formation in supernovae (SNe). To establish the relative importance of these two classes of stellar sources of dust, it is important to know the fract...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2016-03, Vol.587, p.A157
Hauptverfasser:	Bocchio, M., Marassi, S., Schneider, R., Bianchi, S., Limongi, M., Chieffi, A.
Format:	Artikel
Sprache:	eng
Schlagworte:	Asymptotic properties Computing time Dust Ejecta Enrichment extinction galaxies: high-redshift Grains local insterstellar matter Stellar winds Supernovae supernovae: general
Online-Zugang:	Volltext
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