The timing and location of dust formation in the remnant of SN 1987A

The discovery with the Herschel Space Observatory of bright far-infrared and submm emission from the ejecta of the core-collapse supernova SN 1987A has been interpreted as indicating the presence of some 0.4-0.7 M... of dust. We have constructed radiative transfer models of the ejecta to fit optical...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2015-01, Vol.446 (2), p.2089-2101
Hauptverfasser:	Wesson, R., Barlow, M. J., Matsuura, M., Ercolano, B.
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion disks Astronomy Star & galaxy formation Supernovae
Online-Zugang:	Volltext
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