Mergers in Galaxy Groups. II. The Fundamental Plane of Elliptical Galaxies
Dan S. Taranu, John Dubinski, H.K.C. Yee

TL;DR
This study uses simulations of galaxy mergers to show that collisionless processes can produce elliptical galaxies that follow the observed fundamental plane relation, with a tilt mainly caused by increasing dark matter fractions in more massive galaxies.
Contribution
It demonstrates that collisionless mergers can naturally reproduce the fundamental plane and its tilt, highlighting the role of dark matter in galaxy scaling relations.
Findings
Simulated ellipticals lie on a fundamental plane similar to observations.
The tilt of the fundamental plane arises from mass-dependent dark matter fractions.
The scatter in the simulated fundamental plane matches observed tightness.
Abstract
Observations consistently show that elliptical galaxies follow a tight "fundamental plane" scaling relation between size, mean surface brightness and velocity dispersion, with the form . This relation not only has very small (<0.05 dex) intrinsic scatter, but also has significantly different coefficients from the expected virial scaling (a "tilt"). We analyze hundreds of simulations of elliptical galaxies formed from mergers of spiral galaxies in groups to determine if the fundamental plane can emerge from multiple, mostly minor and hierarchical collisionless mergers. We find that these simulated ellipticals lie on a similar fundamental plane with and . The scatter about this plane is not larger than observed, while the tilt is in the correct sense, although is larger than for typical observations. This supports the idea…
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