A new kinematic analysis of broad line emission from QSOs

Details A new kinematic analysis of broad line emission from QSOs A new kinematic analysis of broad line emission from QSOs

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.244..696f&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 244, June 15, 1990, p. 696-700.

Astronomy and Astrophysics

Astronomy

Emission Spectra, Interstellar Gas, Lyman Alpha Radiation, Quasars, Velocity Distribution, Black Holes (Astronomy), Carbon, Molecular Clouds

Scientific paper

A new kinematic analysis of the broad line region in QSOs, demonstrates that it is a necessary consequence of the standard model assuming ballistic outflow that emission lines should be both broad and asymmetric, as observed. Using a number of simplifying assumptions line shapes of C IV in 1330 + 170 and Q0122 - 380 and the general form of Ly-alpha emission are reproduced.

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