The Fundamental Plane for cluster E and S0 galaxies

Abstract

We have analyzed the Fundamental Plane (FP) for a sample of 226 E and S0 galaxies in ten clusters of galaxies. For photometry in Gunn r the best fitting plane is log r_e=1.24 log sigma - 0.82 log <I>_e + cst. The scatter is 0.084 in log r_e. The slope of the FP is not significantly different from cluster to cluster. The residuals of the FP correlate weakly with the velocity dispersion and the surface brightness. Thus, to avoid biases of derived distances the galaxies need to be selected in a homogeneous way. The FP has significant intrinsic scatter. No other structural parameters like ellipticity or isophotal shape can reduce the scatter significantly. The Mg_2-sigma relation differs slightly from cluster to cluster. Galaxies in clusters with lower velocity dispersions have systematically lower Mg_2. With the current stellar population models, it is in best agreement with our results regarding the FP if the offsets are mainly caused by differences in metallicity. Most of the distances that we derive from the FP imply small peculiar motions, <1000km/s. The zero point of the FP must therefore be quite stable. The residuals from the Mg_2-sigma relation may be used to flag galaxies with deviant populations, and possibly to correct the distance determinations for the deviations.

20 pages, gzipped PostScript, 14 figures included. Accepted for publication in MNRAS

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• Morphology, color-magnitude and scaling relations of galaxies in Abell 426
• The Fundamental Plane of Massive Quiescent Galaxies at z~2
• An Oxford SWIFT Integral Field Spectroscopy study of 14 early-type galaxies in the Coma cluster
• The Fundamental Plane in the hierarchical context
• Angular momentum transfer and the size - mass relation in early - type galaxies
• A Lensing View On The Fundamental Plane
• Allan Sandage and the Cosmic Expansion
• The Fundamental Plane Is Not a Plane: Warped Nature of the Fundamental Plane of Early-type Galaxies and Its Implication for Galaxy Formation
• The core fundamental plane of B2 radio galaxies
• A Galaxy X-ray Fundamental Plane?
• The scaling relation of early-type galaxies in clusters. II: Spectroscopic data for galaxies in eight nearby clusters
• The Evolution of Bulge-Dominated Field Galaxies from z~1 to the Present
• Mapping dark matter in the Bullet Cluster using JWST imaging and spectroscopy
• The scaling relations of galaxies back in time: the road toward virialization
• Influence of Cooled Interstellar Gas on the Fundamental Plane for Elliptical Galaxies
• A new framework for understanding the evolution of early-type galaxies
• AstroInspect: a web-based system to organize, assess, and visually inspect astronomical objects
• The Stellar Kinematics of Extragalactic Bulges
• The hyperplane of early-type galaxies: using stellar population properties to increase the precision and accuracy of the fundamental plane as a distance indicator
• Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies: Black Hole Scaling Relations Are Not Biased by Selection Effects
• The Gemini/HST Galaxy Cluster Project: Environment Effects on the Stellar Populations in the Lynx Clusters at z=1.27
• Environmental Effects in the Evolution of Galactic Bulges
• The Fundamental Plane of Elliptical Galaxies in Compact Groups
• Constraints on Galaxy Structure and Evolution from the Light of Nearby Systems
• The bright galaxy population of five medium redshift clusters. II. Quantitative Galaxy Morphology
• The Intergalactic Stellar Population from Mergers of Elliptical Galaxies with Dark Matter halos
• Excursions into the Evolution of Early-Type Galaxies in Clusters
• Using Elliptical Galaxy Kinematics to Compare of the Strength of Gravity in Cosmological Regions of Differing Gravitational Potential -- A First Look
• A Communication Efficient and Scalable Distributed Data Mining for the Astronomical Data
• Dynamical Mass Determinations and Scaling Relations of Early-Type Galaxies
• The velocity dispersion function of red galaxies in four Hubble Frontier Fields galaxy clusters
• Scaling Relations in Dissipationless Spiral-like Galaxy Mergers
• Is there a tilt in the fundamental (hyper)plane?
• Past, present and Future of the Scaling Relations of Galaxies and Active Galactic Nuclei
• Parametric strong lensing model of the galaxy cluster Abell 2390 from Euclid and MUSE observations
• An Extended, Physically Calibrated FP for Elliptical Galaxies
• A SAURON study of stars and gas in Sa bulges
• Clustering around radio galaxies at z~1.5
• VIMOS-IFU survey of z~0.2 massive galaxy clusters. I. Observations of the strong lensing cluster Abell 2667
• Velocity Dispersions and Stellar Populations of the Most Compact and Massive Early-Type Galaxies at Redshift ~1
• The Nature of Galactic Bulges from SAURON Absorption Line Strength Maps