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Whatever happened to the progenitors of supernovae 2008cn, 2009kr and 2009md?★
Author(s) -
J. R. Maund,
M. Fraser,
E. Reilly,
M. Ergon,
S. Mattila
Publication year - 2015
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-8711
pISSN - 0035-8711
DOI - 10.1093/mnras/stu2658
Subject(s) - physics , supernova , astrophysics , supergiant , red supergiant , brightness , flux (metallurgy) , point source , astronomy , stars , optics , materials science , metallurgy
We present new late-time, high-resolution observations of the sites of supernovae (SNe) 2008cn, 2009kr and 2009md, acquired with the Hubble Space Telescope. In all instances, significant flux from the SNe is still recovered at late times. We show that the previous identification of the progenitor of SN 2008cn was actually a blend of two sources, whose locations are resolved in these new observatio...

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