PHYSICAL STRUCTURE AND NATURE OF SUPERNOVA REMNANTS IN M101-Reference-Cited by-同舟云学术

PHYSICAL STRUCTURE AND NATURE OF SUPERNOVA REMNANTS IN M101

Published:2012-03-09 Issue:4 Volume:143 Page:85
ISSN:0004-6256
Container-title:The Astronomical Journal
language:
Short-container-title:The Astronomical Journal

Author:

Franchetti Nicholas A.,Gruendl Robert A.,Chu You-Hua,Dunne Bryan C.,Pannuti Thomas G.,Kuntz Kip D.,Chen C.-H. Rosie,Grimes Caleb K.,Aldridge Tabitha M.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference43 articles.

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

2. The extraordinary extragalactic supernova remnant in NGC 4449. II - X-ray and optical investigations

3. Dense, Fe‐rich Ejecta in Supernova Remnants DEM L238 and DEM L249: A New Class of Type Ia Supernova?

4. [ITAL]HUBBLE SPACE TELESCOPE[/ITAL][ITAL]Hubble Space Telescope[/ITAL] Wide Field Planetary Camera 2 Imaging of Shocks in Superbubbles

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