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Near-IR Properties of Quasar Host Galaxies

K. K. McLeod
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Abstract

We have obtained deep, near-IR images of nearly 100 host galaxies of nearby quasars and Seyferts. We find the near-IR light to be a good tracer of luminous mass in these galaxies. For the most luminous quasars there is a correlation between the maximum allowed B-band nuclear luminosity and the host galaxy mass, a ``luminosity/host-mass limit''. Comparing our images with images from HST, we find that the hosts of these very luminous quasars are likely early type galaxies, even for radio-quiet objects whose lower-luminosity counterparts traditionally live in spirals. We speculate that the luminosity/host-mass limit represents a physical limit on the size of black hole that can exist in a given galaxy spheroid mass. We discuss the promises of NICMOS for detecting the hosts of luminous quasars.

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K. K. McLeod. 1997-01-23. Near-IR Properties of Quasar Host Galaxies. https://arxiv.org/abs/astro-ph/9701185

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