Molecular hydrogen emission from the bright quasar 3C273

Details Molecular hydrogen emission from the bright quasar 3C273 Molecular hydrogen emission from the bright quasar 3C273

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989natur.341..217k&link_type=abstract

Nature (ISSN 0028-0836), vol. 341, Sept. 21, 1989, p. 217, 218. Research supported by the Monbusho International Scientific Rese

Physics

9

Emission Spectra, Hydrogen, Quasars, Seyfert Galaxies, Hubble Constant, Molecular Clouds, Molecular Gases, Polarized Radiation

Scientific paper

Observations of molecular hydrogen emission from the quasar 3C273 are reported. This is the first time such emission has been seen from a radio-loud quasar. The observations support the model of Antonucci and Miller (1985) which holds that the broad emission lines in polarized light observed from type 2 Seyfert galaxies are due to a type 1 Seyfert nucleus shrouded from view by a torus of molecular gas.

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