Optical structure of the accretion disk of HZ Her/Her X-1

Details Optical structure of the accretion disk of HZ Her/Her X-1 Optical structure of the accretion disk of HZ Her/Her X-1

May 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990pazh...16..428a&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 16, May 1990, p. 428-434. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

Accretion Disks, Light Curve, Neutron Stars, Stellar Luminosity, Ubv Spectra, Astronomical Photometry, X Ray Astronomy

Scientific paper

UBV mean light curves of HZ Her were analyzed to elucidate the optical
structure of the accretion disk (AD) surrounding the neutron star. The
AD has a radius that is about 0.6 of the Roche lobe radius of the
neutron star, and the bolometric intensity is 10 to the 35th erg/sec,
which is about 1 percent of the X-ray luminosity.

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