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The peculiar mass-loss history of SN 2014C as revealed through AMI radio observations

Abstract:

We present a radio light curve of supernova (SN) 2014C taken with the Arcminute Microkelvin Imager (AMI) Large Array at 15.7 GHz. Optical observations presented by Milisavljevic et al. demonstrated that SN 2014C metamorphosed from a stripped-envelope Type Ib SN into a strongly interacting Type IIn SN within 1 yr. The AMI light curve clearly shows two distinct radio peaks, the second being a factor of 4 times more luminous than the first peak. This double bump morphology indicates two distinct...

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Publication status:
Published
Peer review status:
Peer reviewed
Version:
Publisher's version

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Publisher copy:
10.1093/mnras/stw3310

Authors


Anderson, GE More by this author
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Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics; Astrophysics
More by this author
Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics; Astrophysics
More by this author
Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics; Astrophysics
Oxford college:
Brasenose College
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Science and Technology Facilities Council More from this funder
Israel Science Foundation More from this funder
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Publisher:
Oxford University Press Publisher's website
Journal:
Monthly Notices of the Royal Astronomical Society Journal website
Volume:
466
Issue:
3
Pages:
3648-3662
Publication date:
2016-12-05
Acceptance date:
2016-12-16
DOI:
EISSN:
1365-2966
ISSN:
0035-8711
Pubs id:
pubs:696570
URN:
uri:6cffdddb-d2a4-448d-aa6d-5165acf00ea9
UUID:
uuid:6cffdddb-d2a4-448d-aa6d-5165acf00ea9
Local pid:
pubs:696570

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