HST UV observations of the accretion disk corona X-ray binary X1822-371

Details HST UV observations of the accretion disk corona X-ray binary X1822-371 HST UV observations of the accretion disk corona X-ray binary X1822-371

Aug 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995adspr..16...65p&link_type=abstract

Advances in Space Research (ISSN 0273-1177), vol. 16, no. 3, p. 65-68

Astronomy and Astrophysics

Astronomy

5

Accretion Disks, Astronomical Models, Coronas, Hubble Space Telescope, Light Curve, X Ray Binaries, Eclipses, Faint Object Camera, Morphology, Temporal Resolution, Ultraviolet Astronomy, Ultraviolet Spectroscopy

Scientific paper

The Faint Object Spectrograph (FOS) on the Hubble Space Telescope (HST) has provided the first ultraviolet orbital light curve of the low-mass X-ray binary X1822-371. The shape of the UV light curve changes with wavelength providing the first direct clues to the temperature of the various system components. The data support the idea that the system contains a thick, structured accretion disk.

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