Rapid formation of large dust grains in the luminous supernova 2010jl

Christa Gall (), Jens Hjorth, Darach Watson, Eli Dwek, Justyn R. Maund, Ori Fox, Giorgos Leloudas, Daniele Malesani and Avril C. Day-Jones
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Christa Gall: Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark
Jens Hjorth: Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, DK-2100 Copenhagen Ø, Denmark
Darach Watson: Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, DK-2100 Copenhagen Ø, Denmark
Eli Dwek: Observational Cosmology Lab, Code 665, NASA Goddard Space Flight Center
Justyn R. Maund: Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, DK-2100 Copenhagen Ø, Denmark
Ori Fox: University of California
Giorgos Leloudas: Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, DK-2100 Copenhagen Ø, Denmark
Daniele Malesani: Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, DK-2100 Copenhagen Ø, Denmark
Avril C. Day-Jones: Universidad de Chile, Camino del Observatorio 1515, Santiago, Chile

Nature, 2014, vol. 511, issue 7509, 326-329

Abstract: The formation of dust in the dense circumstellar medium of the bright supernova 2010jl is at first rapid and produces very large grains, which resist destruction, whereas later the dust production rate increases, meaning its source is ejecta; this links early and late dust mass evolution in supernovae with dense circumstellar media.

Date: 2014
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DOI: 10.1038/nature13558

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