Delayed hard X-rays from Cygnus X-1

Details Delayed hard X-rays from Cygnus X-1 Delayed hard X-rays from Cygnus X-1

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988natur.336..450m&link_type=abstract

Nature (ISSN 0028-0836), vol. 336, Dec. 1, 1988, p. 450-452.

Astronomy and Astrophysics

Astronomy

116

Black Holes (Astronomy), Cygnus Constellation, X Ray Sources, X Ray Spectra, Compton Effect, Cross Correlation, Delay

Scientific paper

Using the large-area proportional counters on the Ginga satellite, the authors have observed Cygnus X-1 in its low state, and complex cross-spectrum analysis of the data reveals that the delay of the high-energy X-rays with respect to the low increases from approximately 2 ms to several seconds for periods from 0.1 to 300 s. This is inconsistent with the inverse Compton scattering model of Cygnus X-1.

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