Optical monitoring of X-ray burst sources

Details Optical monitoring of X-ray burst sources Optical monitoring of X-ray burst sources

Jul 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978mnras.184p..27a&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 184, July 1978, p. 27P-33P.

Astronomy and Astrophysics

Astronomy

2

Astronomical Photometry, Optical Emission Spectroscopy, X Ray Sources, Television Systems, X Ray Astronomy

Scientific paper

Results are presented for simultaneous optical and X-ray observations of the X-ray burst sources MXB 1837+05 and 1916-05. On two occasions during these observations an X-ray burst from MXB 1837+05 was detected by SAS 3, but no accompanying optical signal was detected. The 3-sigma upper limit to the ratio of the energy in a possible optical burst to the energy in the X-ray burst is 0.0001.

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