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Discovery of a Pulsar-Powered Bow Shock Nebula in the Small Magellanic Cloud Supernova Remnant DEM S5

Rami Z. E. Alsaberi,C. Maitra,M. D. Filipovic,L. M. Bozzetto,F. Haberl,P. Maggi, M. Sasaki, P. Manjolovic,V. Velovic,P. Kavanagh,N. I. Maxted,D. Urosevic,G. P. Rowell,G. F. Wong,B-Q For,A. N. O'Brien,T. J. Galvin,L. Staveley-Smith,R. P. Norris,T. Jarrett,R. Kothes,K. J. Luken,N. Hurley-Walker,H. Sano,D. Onic,S. Dai,T. G. Pannuti,N. F. H. Tothill,E. J. Crawford, M. Yew,I. Bojicic,H. Denes,N. McClure-Griffiths,S. Gurovich,Y. Fukui

Monthly Notices of the Royal Astronomical Society（2019）

Cited 17|Views4
Key words
radiation mechanisms: general,ISM: individual objects: DEMS5,ISM: supernova remnants,Magellanic Clouds,radio continuum: ISM
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