Optical Structure and Proper‐Motion Age of the Oxygen‐rich Supernova Remnant 1E 0102−7219 in the Small Magellanic Cloud-Reference-Cited by-同舟云学术

Optical Structure and Proper‐Motion Age of the Oxygen‐rich Supernova Remnant 1E 0102−7219 in the Small Magellanic Cloud

Published:2006-04-20 Issue:2 Volume:641 Page:919-929
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Finkelstein Steven L.,Morse Jon A.,Green James C.,Linsky Jeffrey L.,Shull J. Michael,Snow Theodore P.,Stocke John T.,Brownsberger Kenneth R.,Ebbets Dennis C.,Wilkinson Erik,Heap Sara R.,Leitherer Claus,Savage Blair D.,Siegmund Oswald H.,Stern Alan

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference46 articles.

1. New radio observations of supernova remnant 1E 0102.2-7219 in the Small Magellanic Cloud

2. [ITAL]Hubble Space Telescope[/ITAL] Observations of Proper Motions in Herbig-Haro Objects 1 and 2

3. The ultraviolet spectrum of an oxygen-rich supernova remnant in the Small Magellanic Cloud

4. Hubble Space TelescopeObservations of Oxygen‐rich Supernova Remnants in the Magellanic Clouds. II. Elemental Abundances in N132D and 1E 0102.2−7219

5. Blondin, J. M. 2001, in Young Supernova Remnants, ed. S. S. Holt & U. Hwang (New York: AIP), 59

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