Study of the overall spectrum of the QSO 3C273

Details Study of the overall spectrum of the QSO 3C273 Study of the overall spectrum of the QSO 3C273

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984msngr..37....8c&link_type=abstract

ESO Messenger (ISSN 0722-0091), Sept. 1984, p. 8-10.

Astronomy and Astrophysics

Astronomy

Astronomical Models, Astronomical Spectroscopy, Emission Spectra, Quasars, X Ray Sources, Active Galactic Nuclei, Exosat Satellite, Infrared Spectra, X Ray Spectra

Scientific paper

In order to understand the overall spectra of active galactic nuclei (AGN), the structure of the emission regions was studied. A wind and shock model, developed to explain this structure, is aimed at understanding individual objects such as the quasar QSO 3C 273. The European X-ray satellite EXOSAT, which includes a low energy imaging telescope and a medium energy experiment was used to observe the spectrum of 3C 273 at several wavelengths. The components of the spectrum include the 1R-optical synchroton emission, the thermal component in the optical spectrum, and the comptonized X-ray spectrum.

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