Quantifying the dust in SN 2012aw and iPTF14hls with ORBYTS

Core-collapse supernovae (CCSNe) are capable of producing large quantities of dust, with strong evidence that ejecta dust masses can grow significantly over extended periods of time. Red–blue asymmetries in the broad emission lines of CCSNe can be modelled using the Monte Carlo radiative transfer co...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2023-02, Vol.519 (2), p.2940-2950
Hauptverfasser:	Niculescu-Duvaz, Maria, Barlow, M J, Dunn, William, Bevan, Antonia, Ahmed, Omar, Arkless, David, Barker, Jon, Bartolotta, Sidney, Brockway, Liam, Browne, Daniel, Esmail, Ubaid, Garner, Max, Guz, Wiktoria, King, Scarlett, Kose, Hayri, Lampstaes-Capes, Madeline, Magen, Joseph, Morrison, Nicole, Oo, Kyaw, Paik, Balvinder, Primrose, Joanne, Quick, Danny, Radeka, Anais, Rodney, Anthony, Sandeman, Eleanor, Sheikh, Fawad, Stansfield, Camron, Symister, Delayne, Taylor, Joshua, Wilshere, William, Wesson, R, De Looze, I, Clayton, G C, Krafton, K, Matsuura, M
Format:	Artikel
Sprache:	eng
Online-Zugang:	Volltext
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