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2020ApJ...895...60R - Astrophys. J., 895, 60-60 (2020/May-3)
Discovery of a 28 s pulsar in a 2 day orbit high-mass X-ray binary powering the ultraluminous X-ray source ULX-7 in M51.
RODRIGUEZ CASTILLO G.A., ISRAEL G.L., BELFIORE A., BERNARDINI F., ESPOSITO P., PINTORE F., DE LUCA A., PAPITTO A., STELLA L., TIENGO A., ZAMPIERI L., BACHETTI M., BRIGHTMAN M., CASELLA P., D'AGOSTINO D., DALL'OSSO S., EARNSHAW H.P., FURST F., HABERL F., HARRISON F.A., MAPELLI M., MARELLI M., MIDDLETON M., PINTO C., ROBERTS T.P., SALVATERRA R., TUROLLA R., WALTON D.J. and WOLTER A.
Abstract (from CDS):
Abstract Copyright: © 2020. The American Astronomical Society. All rights reserved.
Journal keyword(s): Neutron stars - Stellar accretion - X-ray sources - Stellar magnetic fields - X-ray binary stars - Pulsars
Simbad objects: 17
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