Optically thin thermal emission as the origin of the big bump in the spectra of active galactic nuclei

Details Optically thin thermal emission as the origin of the big bump in the spectra of active galactic nuclei Optically thin thermal emission as the origin of the big bump in the spectra of active galactic nuclei

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...363l..21f&link_type=gif

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 363, Nov. 10, 1990, p. L21-L25.

Astronomy and Astrophysics

Astrophysics

99

Active Galactic Nuclei, Markarian Galaxies, Optical Thickness, Seyfert Galaxies, Thermal Emission, Astronomical Spectroscopy, Balmer Series, Line Spectra, Ultraviolet Radiation, X Ray Spectra

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