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Contribution to a conference proceedings/Contribution to a book | PUBDB-2016-05625 |
2016
Verlag Deutsches Elektronen-Synchrotron
Hamburg
ISBN: 978-3-945931-08-0
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Please use a persistent id in citations: doi:10.3204/DESY-PROC-2016-05/35
Abstract: Observing the evolution of a supernova over several decades is unique. SN~1987A is the only object where this has been possible in great detail and it has shown us some physics, which we never had expected. Even now - after 10000 days - does SN~1987A provide new surprises on its way to become a supernova remnant. We present here an overview of the current status of the observations of SN~1987A with a focus on the evolution of the emission from the circumstellar ring. SN~1987A can be detected at all electromagnetic wavelengths, which gives us a complete picture of the energy sources and some of the radiation transfer. There are several emission sites present in SN~1987A and we will present them in this overview.
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Book/Proceedings/Report
Proceedings, Magellan Workshop : Connecting Neutrino Physics and Astronomy : Hamburg, Germany, March 17-18, 2016
Magellan Workshop, HamburgHamburg, Germany, 17 Mar 2016 - 18 Mar 2016
Hamburg : Verlag Deutsches Elektronen-Synchrotron, DESY-PROC 1-228 (2016) [10.3204/DESY-PROC-2016-05]
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