Comparisons between X-ray variabilities from the Sun, GRB and X-ray binaries

Details Comparisons between X-ray variabilities from the Sun, GRB and X-ray binaries Comparisons between X-ray variabilities from the Sun, GRB and X-ray binaries

Jan 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc..968..392t&link_type=abstract

ASTROPHYSICS OF COMPACT OBJECTS: International Conference on Astrophysics of Compact Objects. AIP Conference Proceedings, Volum

Astronomy and Astrophysics

Astrophysics

X-Ray Binaries, Flares, Gamma-Ray Sources, Gamma-Ray Bursts

Scientific paper

We investigate the X-ray variabilities from the Sun, GRB and X-ray binaries. The net X-ray RMS from the Sun shows a linear dependence on the X-ray flux, over a dynamical range of several orders of magnitudes [1]. In many cases, similar X-ray variability is also seen from X-ray binaries [3] and a GRB, albeit within smaller dynamical ranges of flux variations. Such X-ray variabilities may be produced by many X-ray emission nodes inter-connected by large scale magnetic fields. Millisecond variability from a black hole X-ray binary has also been observed sometimes, but the variability can be described by random superposititons of independent millisecond shots.

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