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）
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radiation mechanisms: general,ISM: individual objects: DEMS5,ISM: supernova remnants,Magellanic Clouds,radio continuum: ISM
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