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1998A&A...333L..55C - Astronomy and Astrophysics, volume 333L55-58 (1998/5-2)
Detection of an X-ray pulsed signal from the supernova remnant N157B in the Large Magellanic Cloud.
CUSUMANO G., MACCARONE M.C., MINEO T., SACCO B., MASSARO E., BANDIERA R. and SALVATI M.
Abstract (from CDS):
The supernova remnant N157B was in the field of view during an observation of the LMC with the BeppoSAX satellite. A signal with a 16 ms periodicity was detected in the MECS data. The pulse profile is characterized by a single narrow peak with a flux of (5.1±1.1)x10–13erg/cm2/s. In this paper the dynamical state of the plerion-shell system is discussed, and inferences are drawn on the optical luminosity of the pulsar and the plerion.
Abstract Copyright: ∼
Journal keyword(s): stars - stars: neutron - pulsars: individual - X-rays: stars
Simbad objects: 7
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