One Big Monster or Many Little Beasties?

Details One Big Monster or Many Little Beasties? One Big Monster or Many Little Beasties?

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1201..206s&link_type=abstract

THE MONSTER'S FIERY BREATH: FEEDBACK IN GALAXIES, GROUPS, AND CLUSTERS. AIP Conference Proceedings, Volume 1201, pp. 206-209 (2

Physics

Galactic Nuclei, X-Ray Emission Spectra, Galaxies, Clusters Of Galaxies, Brightness, Galactic Nuclei, Circumnuclear Matter, And Bulges, X-Ray, Elliptical Galaxies, Galaxy Clusters, Magnitudes And Colors, Luminosities

Scientific paper

Following the Hart et al. contribution to this volume, we use the results of her survey to speculate that: (1) Virtually all bright cluster red sequence (CRS) elliptical galaxies in the inner regions (<=500 kpc from the center) of rich clusters are low-luminosity BL Lac Objects with relativistic jets; (2) These low-luminosity AGN may dominate the heat input into the intracluster medium; and (3) While Bondi accretion of ICM gas can explain the central concentration of these AGN, several aspects of non-BCG AGN cast doubt on whether or not gas accretion powers these sources.

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