SN1987A: The X-ray remnant at age 25 years

David N. Burrows; Sangwook Park; Eveline A. Helder; Daniel Dewey; Richard McCray; Svetozar A. Zhekov; Judith L. Racusin; Eli Dwek

doi:10.1017/S1743921312012719

SN1987A: The X-ray remnant at age 25 years

David N. Burrows
, Sangwook Park
, Eveline A. Helder
, Daniel Dewey
, Richard McCray
, Svetozar A. Zhekov
, Judith L. Racusin
, Eli Dwek

Astronomy & Astrophysics

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Abstract

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.

Original language	English (US)
Title of host publication	Death of Massive Stars
Subtitle of host publication	Supernovae and Gamma-Ray Bursts
Editors	Peter W. A. San Antonio, Nobuyuki Kawai, Elena Pian
Pages	71-74
Number of pages	4
Edition	S279
DOIs	https://doi.org/10.1017/S1743921312012719
State	Published - Apr 2011

Publication series

Name	Proceedings of the International Astronomical Union
Number	S279
Volume	7
ISSN (Print)	1743-9213
ISSN (Electronic)	1743-9221

UN SDGs

This output contributes to the following UN Sustainable Development Goals (SDGs)

SDG 3 Good Health and Well-being

All Science Journal Classification (ASJC) codes

Medicine (miscellaneous)
Astronomy and Astrophysics
Nutrition and Dietetics
Public Health, Environmental and Occupational Health
Space and Planetary Science

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10.1017/S1743921312012719

Cite this

Burrows, D. N., Park, S., Helder, E. A., Dewey, D., McCray, R., Zhekov, S. A., Racusin, J. L., & Dwek, E. (2011). SN1987A: The X-ray remnant at age 25 years. In P. W. A. San Antonio, N. Kawai, & E. Pian (Eds.), Death of Massive Stars: Supernovae and Gamma-Ray Bursts (S279 ed., pp. 71-74). (Proceedings of the International Astronomical Union; Vol. 7, No. S279). https://doi.org/10.1017/S1743921312012719

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title = "SN1987A: The X-ray remnant at age 25 years",

abstract = "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.",

author = "Burrows, \{David N.\} and Sangwook Park and Helder, \{Eveline A.\} and Daniel Dewey and Richard McCray and Zhekov, \{Svetozar A.\} and Racusin, \{Judith L.\} and Eli Dwek",

year = "2011",

month = apr,

doi = "10.1017/S1743921312012719",

language = "English (US)",

isbn = "9781107019799",

series = "Proceedings of the International Astronomical Union",

number = "S279",

pages = "71--74",

editor = "\{San Antonio\}, \{Peter W. A.\} and Nobuyuki Kawai and Elena Pian",

booktitle = "Death of Massive Stars",

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}

Burrows, DN, Park, S, Helder, EA, Dewey, D, McCray, R, Zhekov, SA, Racusin, JL & Dwek, E 2011, SN1987A: The X-ray remnant at age 25 years. in PWA San Antonio, N Kawai & E Pian (eds), Death of Massive Stars: Supernovae and Gamma-Ray Bursts. S279 edn, Proceedings of the International Astronomical Union, no. S279, vol. 7, pp. 71-74. https://doi.org/10.1017/S1743921312012719

SN1987A: The X-ray remnant at age 25 years. / Burrows, David N.; Park, Sangwook; Helder, Eveline A. et al.
Death of Massive Stars: Supernovae and Gamma-Ray Bursts. ed. / Peter W. A. San Antonio; Nobuyuki Kawai; Elena Pian. S279. ed. 2011. p. 71-74 (Proceedings of the International Astronomical Union; Vol. 7, No. S279).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

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AU - Burrows, David N.

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AU - Zhekov, Svetozar A.

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AB - 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.

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A2 - San Antonio, Peter W. A.

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ER -

SN1987A: The X-ray remnant at age 25 years

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