Synchrotron Self-Compton Models for Superluminal Radio Sources, Periodic Variability and Complex Absorption in the Seyfert Galaxy NGC6814, and Soft X-Ray Properties of a Complete Radio-Selected Sample of BL Lacertae Objects

Details Synchrotron Self-Compton Models for Superluminal Radio Sources, Periodic Variability and Complex Absorption in the Seyfert Galaxy NGC6814, and Soft X-Ray Properties of a Complete Radio-Selected Sample of BL Lacertae Objects Synchrotron Self-Compton Models for Superluminal Radio Sources, Periodic Variability and Complex Absorption in the Seyfert Galaxy NGC6814, and Soft X-Ray Properties of a Complete Radio-Selected Sample of BL Lacertae Objects

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996stsc.reptq....u&link_type=abstract

Technical Report, Space Telescope Science Inst. Baltimore, MD United States

Astronomy and Astrophysics

Astronomy

Bl Lacertae Objects, Seyfert Galaxies, X Ray Astronomy, Radio Astronomy, Astronomical Models, Radio Sources (Astronomy), Synchrotrons, Variability, Stellar Luminosity, Compton Effect, X Rays

Scientific paper

Considerable progress has been made on the project to understand the X-ray properties of radio-selected BL Lacertae Objects. A large number of related papers have been published or accepted for publication, and are listed in this report along with conference submissions and book chapters. The grant extended to 'Synchrotron Self-Compton Models for Superluminal Radio Sources' and 'Periodic Variability and Complex Absorption in the Seyfert Galaxy NGC 6814.'

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