THE INFLUENCE OF SUPERNOVA REMNANTS ON THE INTERSTELLAR MEDIUM IN THE LARGE MAGELLANIC CLOUD SEEN AT 20-600 μm WAVELENGTHS-Reference-Cited by-同舟云学术

THE INFLUENCE OF SUPERNOVA REMNANTS ON THE INTERSTELLAR MEDIUM IN THE LARGE MAGELLANIC CLOUD SEEN AT 20-600 μm WAVELENGTHS

Published:2015-01-14 Issue:1 Volume:799 Page:50
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Lakićević Maša^ORCID,van Loon Jacco Th.,Meixner Margaret,Gordon Karl^ORCID,Bot Caroline,Roman-Duval Julia^ORCID,Babler Brian^ORCID,Bolatto Alberto,Engelbracht Chad,Filipović Miroslav^ORCID,Hony Sacha,Indebetouw Remy,Misselt Karl,Montiel Edward,Okumura K.,Panuzzo Pasquale,Patat Ferdinando,Sauvage Marc,Seale Jonathan,Sonneborn George^ORCID,Temim Tea,Urošević Dejan,Zanardo Giovanna^ORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.1088/0004-637X/799/1/50/pdf

Reference99 articles.

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3. SPITZEROBSERVATIONS OF DUST DESTRUCTION IN THE PUPPIS A SUPERNOVA REMNANT

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

5. On the size distribution of supernova remnants in the Magellanic Clouds

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