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arXiv · astro-ph/0412123

Dynamical models linking BH masses and DM content

Pieter Buyle·Herwig Dejonghe·Maarten Baes
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Abstract

We investigate the relation between the dark matter distribution of galaxies and their central supermassive black holes which is suggested by the v_c-sigma relation. Since early-type galaxies appear to have larger black holes than late-type ones, we look for an equivalent pattern in the dark matter distribution as a function of Hubble type. To achieve our goal we use a state-of-the-art modelling code that allows a variety of geometries to be fitted to a combination of radio and optical observations of galaxies with different morphology.

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Pieter Buyle, Herwig Dejonghe, Maarten Baes. 2004-12-06. Dynamical models linking BH masses and DM content. https://doi.org/10.1007/11403913_31

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