The slope of the mass profile and the tilt of the fundamental plane in early-type galaxies
Philip J. Humphrey, David A. Buote (UC Irvine)

TL;DR
This study uses Chandra X-ray data to analyze mass profiles in galaxies, revealing a systematic variation in density slopes that explains the fundamental plane tilt through baryonic and dark matter interplay.
Contribution
It demonstrates that the total mass distribution in early-type galaxies follows a powerlaw profile with a slope varying systematically with galaxy size, linking it to the fundamental plane tilt.
Findings
Mass density profiles are close to powerlaws from 0.2 to 10 Re.
The slope alpha varies from 2 to 1.2 with galaxy size.
Dark matter fraction within Re correlates with galaxy properties.
Abstract
We present a survey, using the Chandra X-ray observatory, of the central gravitating mass profiles in a sample of 10 galaxies, groups and clusters, spanning ~2 orders of magnitude in virial mass. We find the total mass distributions from ~0.2--10Re, where Re is the optical effective radius of the central galaxy, are remarkably similar to powerlaw density profiles. The negative logarithmic slope of the mass density profiles, alpha, systematically varies with Re, from alpha=2, for systems with Re~4kpc to alpha=1.2 for systems with Re>30kpc. Departures from hydrostatic equilibrium are likely to be small and cannot easily explain this trend. We show that the conspiracy between the baryonic (Sersic) and dark matter (NFW/ Einasto) components required to maintain a powerlaw total mass distribution naturally predicts an anti-correlation between alpha and Re that is very close to what is…
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