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2020MNRAS.498.4705V - Mon. Not. R. Astron. Soc., 498, 4705-4720 (2020/November-2)
Be X-ray binaries in the SMC as indicators of mass-transfer efficiency.
VINCIGUERRA S., NEIJSSEL C.J., VIGNA-GOMEZ A., MANDEL I., PODSIADLOWSKI P., MACCARONE T.J., NICHOLL M., KINGDON S., PERRY A. and SALEMI F.
Abstract (from CDS):
Abstract Copyright: © 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal keyword(s): X-rays: binaries - stars: emission-line, Be - stars: neutron - stars: evolution - gravitational waves - methods: data analysis
Simbad objects: 6
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