Dependence of the Fundamental Plane of Early-type Galaxies on Age and Internal Structure

Abstract

We investigate the scatter in the fundamental plane (FP) of early-type galaxies (ETGs) and its dependence on age and internal structure of ETGs, using $16,283$ ETGs with $M_r\le -19.5$ and $0.025\le z<0.055$ in Sloan Digital Sky Survey data. We use the relation between the age of ETGs and photometric parameters such as color, absolute magnitude, and central velocity dispersion of ETGs and find that the scatter in the FP depends on age. The FP of old ETGs with age $\gtrsim 9$ Gyrs has a smaller scatter of $\sim 0.06$ dex ($\sim 14\%$) while that of young ETGs with age $\lesssim 6$ Gyrs has a larger scatter of $\sim 0.075$ dex ($\sim 17\%$). In the case of young ETGs, less compact ETGs have a smaller scatter in the FP ($\sim 0.065$ dex; $\sim 15\%$) than more compact ones ($\sim 0.10$ dex; $\sim 23\%$). On the other hand, the scatter in the FP of old ETGs does not depend on the compactness of galaxy structure. Thus, among the subpopulations of ETGs, compact young ETGs have the largest scatter in the FP. This large scatter in compact young ETGs is caused by ETGs that have low dynamical mass-to-light ratio ($M_{\mathrm{dyn}}/L$) and blue color in the central regions. By comparing with a simple model of the galaxy that has experienced a gas-rich major merger, we find that the scenario of recent gas-rich major merger can reasonably explain the properties of the compact young ETGs with excessive light for a given mass (low $M_{\mathrm{dyn}}/L$) and blue central color.

17 pages, 12 figures, 4 tables, accepted for publication in the ApJ

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• How to empirically model star formation in dark matter halos: I. Inferences about central galaxies from numerical simulations
• The Fundamental Plane Is Not a Plane: Warped Nature of the Fundamental Plane of Early-type Galaxies and Its Implication for Galaxy Formation
• The hyperplane of early-type galaxies: using stellar population properties to increase the precision and accuracy of the fundamental plane as a distance indicator
• Late growth of early-type galaxies in low-z massive clusters
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