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2019MNRAS.486.2507A - Mon. Not. R. Astron. Soc., 486, 2507-2524 (2019/June-3)
Discovery of a pulsar-powered bow shock nebula in the Small Magellanic Cloud supernova remnant DEM S5.
ALSABERI R.Z.E., MAITRA C., FILIPOVIC M.D., BOZZETTO L.M., HABERL F., MAGGI P., SASAKI M., MANJOLOVIC P., VELOVIC V., KAVANAGH P., MAXTED N.I., UROSEVIC D., ROWELL G.P., WONG G.F., FOR B.-Q., O'BRIEN A.N., GALVIN T.J., STAVELEY-SMITH L., NORRIS R.P., JARRETT T., KOTHES R., LUKEN K.J., HURLEY-WALKER N., SANO H., ONIC D., DAI S., PANNUTI T.G., TOTHILL N.F.H., CRAWFORD E.J., YEW M., BOJICIC I., DENES H., McCLURE-GRIFFITHS N., GUROVICH S. and FUKUI Y.
Abstract (from CDS):
Abstract Copyright: © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal keyword(s): radiation mechanisms: general - ISM: individual objects: DEM S5 - ISM: supernova remnants - Magellanic Clouds - radio continuum: ISM
Status at CDS : Examining the need for a new acronym.
Simbad objects: 37
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