The EXOSAT observations of the X-ray source in the globular cluster Terzan 2

Details The EXOSAT observations of the X-ray source in the globular cluster Terzan 2 The EXOSAT observations of the X-ray source in the globular cluster Terzan 2

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985esasp.236..263b&link_type=abstract

In ESA Recent Results on Cataclysmic Variables p 263-265 (SEE N86-20287 10-93)

Computer Science

Exosat Satellite, Globular Clusters, X Ray Sources, Accretion Disks, Stellar Luminosity, Stellar Models, Stellar Spectra

Scientific paper

The Globular Cluster X-ray source 4U1722-30 was observed with EXOSAT on 1985 March 14. The observed spectrum and the luminosity, 3.8 times 10 to the 36th power erg/sec, are consistent with Einstein observations of this source. No long term or burst temporal variability are apparent during the 11 hr of observation, but shot noise with typical time scale of 3.5 sec is revealed by autocorrelation analysis. The result is relevant in the context of the models proposed for accretion disks around the compact component in interacting binary systems.

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