Starburst-black hole QSO model. I - Broad emission lines and the central luminosity

Details Starburst-black hole QSO model. I - Broad emission lines and the central luminosity Starburst-black hole QSO model. I - Broad emission lines and the central luminosity

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aipc..254..548d&link_type=abstract

In: Testing the AGN paradigm; Proceedings of the 2nd Annual Topical Astrophysics Conference, Univ. of Maryland, College Park, Oc

Astronomy and Astrophysics

Astronomy

8

Accretion Disks, Black Holes (Astronomy), Interstellar Matter, Luminosity, Quasars, Spectral Line Width, Star Clusters, Compton Effect, Emission Spectra, Seyfert Galaxies, Stellar Mass Ejection

Scientific paper

Accurate stellar evolution tracks are employed to model a wide range of starburst clusters. Mass loss from a cluster with 10 exp 9 solar masses can easily generate an accretion luminosity of about 10 exp 47 ergs/s. The SNR is about 1 per year, as required to create the high ionization lines (HILs). The mass of HIL gas is a few MSN, as inferred from observations.

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