AN X-RAY STUDY OF SUPERNOVA REMNANT N49 AND SOFT GAMMA-RAY REPEATER 0526-66 IN THE LARGE MAGELLANIC CLOUD-Reference-Cited by-同舟云学术

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AN X-RAY STUDY OF SUPERNOVA REMNANT N49 AND SOFT GAMMA-RAY REPEATER 0526-66 IN THE LARGE MAGELLANIC CLOUD

Published:2012-03-14 Issue:2 Volume:748 Page:117
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Park Sangwook,Hughes John P.,Slane Patrick O.,Burrows David N.,Lee Jae-Joon,Mori Koji

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/748/i=2/a=117/pdf

Reference50 articles.

1. Abundances of the elements: Meteoritic and solar

2. Discovery of explosion fragments outside the Vela supernova remnant shock-wave boundary

3. Constraints on the Physics of Type Ia Supernovae from the X‐Ray Spectrum of the Tycho Supernova Remnant

4. THE STELLAR ANCESTRY OF SUPERNOVAE IN THE MAGELLANIC CLOUDS. I. THE MOST RECENT SUPERNOVAE IN THE LARGE MAGELLANIC CLOUD

5. Supernova Remnants Associated with Molecular Clouds in the Large Magellanic Cloud

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