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PHOTOMETRIC AND SPECTROSCOPIC EVOLUTION OF THE IIP...
Journal article

PHOTOMETRIC AND SPECTROSCOPIC EVOLUTION OF THE IIP SN 2007it TO DAY 944

Abstract

SN 2007it is a bright, Type IIP supernova which shows indications of both pre-existing and newly formed dust. The visible photometry shows a bright late-time luminosity, powered by the 0.09 M☉ of 56Ni present in the ejecta. There is also a sudden drop in optical brightness after day 339, and a corresponding brightening in the IR due to new dust forming in the ejecta. CO and SiO emission, generally thought to be precursors to dust formation, may …

Authors

Andrews JE; Sugerman BEK; Clayton GC; Gallagher JS; Barlow MJ; Clem J; Ercolano B; Fabbri J; Meixner M; Otsuka M

Journal

The Astrophysical Journal, Vol. 731, No. 1,

Publisher

American Astronomical Society

Publication Date

April 10, 2011

DOI

10.1088/0004-637x/731/1/47

ISSN

0004-637X