Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.193...15l&link_type=abstract
Monthly Notices of the Royal Astronomical Society, vol. 193, Oct. 1980, p. 15-28.
Astronomy and Astrophysics
Astronomy
40
Spaceborne Astronomy, X Ray Sources, X Ray Stars, Astronomical Models, Bursts, Radiant Flux Density, Sas-3, Statistical Correlation, Time Response
Scientific paper
The paper discusses the SAS-3 X-ray observations of MXB 1735-44 during 1977-78. Fifty-three bursts were observed in 20 days, in irregular intervals from 2 to more than 50 hr. The irregular burst behavior of MXB 1735-44 may be caused by its high intrinsic X-ray luminosity. No correlations were found between burst frequency and properties of the associated persistent source, such as flux and hardness of the persistent spectrum. There may be a correlation between the size of the bursts and burst intervals: the bursts tend to be smaller when they occur more frequently. The distributions of the burst sizes in terms of their integrated burst flux and maximum burst flux have standard deviations of about 37%.
Cominsky Lynn
Holzner S.
Lewin Walter H. G.
Paradijs Jan van
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