Some further information on the rapid burster MXB 1730-335

Details Some further information on the rapid burster MXB 1730-335 Some further information on the rapid burster MXB 1730-335

May 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...214l..11u&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 214, May 15, 1977, p. L11-L15.

Astronomy and Astrophysics

Astrophysics

19

Binary Stars, Satellite Observation, Variable Stars, X Ray Sources, Bursts, Fourier Analysis, High Resolution, Neutron Stars, Sas-3, Sequential Analysis, X Ray Scattering

Scientific paper

Further analysis of SAS-3 data on the rapid burster MXB 1730-335 show the existence of anomalous bursts. They have approximately 3-s rise times and low peak intensities; they also violate the energy vs. interburst-interval relationship for normal bursts. The short normal bursts of about 4-s duration do not show a long tail such as observed in the long normal bursts. Evidence for time structure in normal bursts down to a time scale of 50 ms is presented. No periodic variations in the total X-ray flux were found in the 1-500-Hz range.

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