The accretion matter at the disk rim in HER X-1/HZ HER

Details The accretion matter at the disk rim in HER X-1/HZ HER The accretion matter at the disk rim in HER X-1/HZ HER

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.154..189b&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 154, no. 2, April 1989, p. 189-200.

Astronomy and Astrophysics

Astronomy

13

Accretion Disks, Astronomical Photometry, Light Curve, Stellar Mass Accretion, X Ray Binaries, Astronomical Models, Astronomical Spectroscopy, Linear Polarization, Polarimetry, Ultraviolet Astronomy, Visible Spectrum

Scientific paper

Certain photometric and polarimetric features of the emission from Her X-1, are analyzed, and an empirical model for a blob is constructed. Physical reasons are given for the blob persistence and evolution. The model makes it possible to interpret diverse observational data on blob matter and to make predictions of observational manifestations in the optical, UV, and X-ray bands. The first results of optical spectrum observations of blobs are described.

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