Ejecta, dust, and synchrotron radiation in SNR B0540-69.3: A more crab-like remnant than the crab

Astrophysical Journal

Volumn 687, Issue 2, 2008, Pages 1054-1069

  Williams, Brian J ^a   Borkowski, Kazimierz J ^a   Reynolds, Stephen P ^a   Raymond, John C ^b   Long, Knox S ^c   Morse, Jon ^d   Blair, William P ^e   Ghavamian, Parviz ^e   Sankrit, Ravi ^f   Hendrick, Sean P ^g   Smith, R Chris ^h   Points, Sean ^h   Winkler, P Frank ⁱ  

^a NORTH CAROLINA STATE UNIVERSITY   (United States)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^c STScI   (United States)

^d NASA GODDARD SPACE FLIGHT CENTER   (United States)

^e JOHNS HOPKINS UNIVERSITY   (United States)

^f UNIVERSITY OF CALIFORNIA   (United States)

^g MILLERSVILLE UNIVERSITY   (United States)

^h CERRO TOLOLO INTER AMERICAN OBSERVATORY   (Chile)

ⁱ MIDDLEBURY COLLEGE   (United States)

Author keywords

Dust, extinction; Magellanic clouds; Pulsars: individual (SNR 0540 69.3); Supernova remnants

Indexed keywords

EID: 55849095835     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/592139     Document Type: Article

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