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SN1987A: the X-ray remnant at age 25 years

Published online by Cambridge University Press:  05 September 2012

David N. Burrows ,
Sangwook Park ,
Eveline A. Helder ,
Daniel Dewey ,
Richard McCray ,
Svetozar A. Zhekov ,
Judith L. Racusin  and
Eli Dwek
David N. Burrows
Affiliation:
Dept. of Astronomy & Astrophysics, Penn State University, University Park, PA 16802USA; email: [email protected];
Sangwook Park
Affiliation:
U. Texas-Arlington, Arlington, TX, USA;
Eveline A. Helder
Affiliation:
Dept. of Astronomy & Astrophysics, Penn State University, University Park, PA 16802USA; email: [email protected];
Daniel Dewey
Affiliation:
MIT Kavli Institute, Cambridge, MA, USA
Richard McCray
Affiliation:
U. Colorado, Boulder, CO, USA;
Svetozar A. Zhekov
Affiliation:
Space Research and Technology Institute, Sofia, Bulgaria
Judith L. Racusin
Affiliation:
NASA/GSFC, Greenbelt, MD, USA
Eli Dwek
Affiliation:
NASA/GSFC, Greenbelt, MD, USA
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Abstract

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SN1987A is the best-studied core-collapse supernova in the sky. We know what the progenitor was, what the circumstellar environment was, and what the explosion looked like over a broad electromagnetic bandpass and in neutrinos. For over a decade, the Chandra X-ray Observatory has been monitoring SN1987A on a regular basis, obtaining resolved images of the developing interaction with the circumstellar material, as well as high resolution grating spectroscopy of the X-ray emission. We highlight the latest results from this campaign and discuss the overall picture of the remnant's structure that emerges from these observations.

Keywords

X-rays:individual(SN1987A)stars:supernovae:individual(SN1987A)
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S279: Death of Massive Stars: Supernovae and Gamma-Ray Bursts , April 2011 , pp. 71 - 74
Copyright
Copyright © International Astronomical Union 2012

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