The detection of far-ultraviolet line emission from balmer-dominated supernova remnants in the Large Magellanic Cloud

Astrophysical Journal

Volumn 664, Issue 1 I, 2007, Pages 304-321

  Ghavamian, Parviz ^a   Blair, William P ^a   Sankrit, Ravi ^b   Raymond, John C ^c   Hughes, John P ^d  

^a JOHNS HOPKINS UNIVERSITY   (United States)

^b UNIVERSITY OF CALIFORNIA   (United States)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^d RUTGERS UNIVERSITY   (United States)

Author keywords

ISM: individual (SNR 0505 67.9 DEM L 71 , SNR 0509 67.5, SNR 0519 69.0, SNR 0548 70.4); ISM: kinematics and dynamics; Shock waves; Supernova remnants

Indexed keywords

EID: 34547685908     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/518686     Document Type: Article

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