The Fundamental Scaling Relations of Elliptical Galaxies
B. Robertson (1), T. J. Cox (1), L. Hernquist (1), M. Franx (2), P. F., Hopkins (1), P. Martini (3), and V. Springel (4) ((1) Harvard/CfA, (2) Leiden, Observatory, (3) OSU, (4) MPA-Garching)

TL;DR
This study investigates how gas dissipation and progenitor properties influence the scaling relations of elliptical galaxies formed through mergers, highlighting the role of gas content and black hole feedback in shaping the Fundamental Plane.
Contribution
It demonstrates that gas dissipation significantly affects the tilt of the Fundamental Plane and provides detailed simulation-based insights into the structural origins of galaxy scaling relations.
Findings
Gas dissipation increases the tilt of the Fundamental Plane.
Higher gas fractions (>30%) lead to scalings matching observations.
Black hole feedback has minor effects on stellar-mass relations.
Abstract
(ABRIDGED) We examine the fundamental scaling relations of elliptical galaxies formed through mergers. Using hundreds of simulations to judge the impact of progenitor galaxy properties on merger remnants, we find that gas dissipation provides an important contribution to tilt in the Fundamental Plane relation. Dissipationless mergers of disks produce remnants that occupy the virial plane. As the gas content of disk galaxies is increased, the tilt of the Fundamental Plane relation increases and the slope of the Re-M_* relation steepens. For gas fractions fgas > 30%, the simulated Fundamental Plane scalings approach those observed in the K-band. In our simulations, feedback from supermassive black hole growth has only a minor influence on the stellar-mass scaling relations of spheroidal galaxies, but may play a role in maintaining the observed Fundamental Plane tilt at optical wavelengths…
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Galaxies: Formation, Evolution, Phenomena · Cosmology and Gravitation Theories
