Erratic variability in mxb 1916-05

Details Erratic variability in mxb 1916-05 Erratic variability in mxb 1916-05

May 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984aipc..115...80h&link_type=abstract

AIP Conference Proceedings, Volume 115, pp. 80-82 (1984).

Physics

X-Ray Sources, X-Ray Bursts, X-Ray Binaries, Neutron Stars, X-Ray

Scientific paper

Five day light curves of MXB 1916-05 obtained 6 month apart reveal two modes of behavior. In the fall 1977 the source had several extended periods of low flux as well as generally erratic variability. In the Spring 1978 the flux steadily increased over several days. The 50 minute period was not detected. We interpret the erratic variability as an instability in the accretion disk.

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