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2021MNRAS.504..326M - Mon. Not. R. Astron. Soc., 504, 326-337 (2021/June-2)
XMMU J050722.1-684758: discovery of a new Be X-ray binary pulsar likely associated with the supernova remnant MCSNR J0507-6847.
MAITRA C., HABERL F., MAGGI P., KAVANAGH P.J., VASILOPOULOS G., SASAKI M., FILIPOVIC M.D. and UDALSKI A.
Abstract (from CDS):
Abstract Copyright: © 2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society
Journal keyword(s): Radiation mechanisms: general - ISM: supernova remnants - Magellanic Clouds - Radio continuum: ISM - X-rays: individuals: XMMU J050722.1-684758 - X-rays: individuals: MCSNR J0507-6847
Simbad objects: 19
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