Toward Understanding the origin of the Fundamental Plane for Early-Type Galaxies
arXiv:astro-ph/0606400 · doi:10.1016/j.newar.2006.03.001
Abstract
We present a panoramic review of several observational and theoretical aspects of the modern astrophysical research about the origin of the Fundamental Plane (FP) relation for Early-Type Galaxies (ETGs). The discussion is focused on the problem of the tilt and the tightness of the FP, and on the attempts to derive the luminosity evolution of ETGs with redshift. Finally, a number of observed features in the FP are interpreted from the standpoint of a new theoretical approach based on the two-component tensor virial theorem.
30 pages, 3 figures
References in corpus (66)
- Dark Matter Substructure in Galactic Halos
- The Inner Structure of LambdaCDM Halos III: Universality and Asymptotic Slopes
- The Inner Structure of LambdaCDM Halos I: A Numerical Convergence Study
- Resolving the Structure of Cold Dark Matter Halos
- On the shape of the light profiles of early-type galaxies
- Analytical Models For Galactic Nuclei
- The Fundamental Plane for cluster E and S0 galaxies
- HST photometry of dwarf elliptical galaxies in Coma, and an explanation for the alleged structural dichotomy between dwarf and bright elliptical galaxies
- The Ages of Elliptical Galaxies in a Merger Model
- Early-type galaxies in the SDSS. III. The Fundamental Plane
- The Phase-Space Density Profiles of Cold Dark Matter Halos
- The Dark Matter Distribution in the Central Regions of Galaxy Clusters: Implications for CDM
- The Dark Matter Distribution in the Central Regions of Galaxy Clusters
- Early-type galaxies in the SDSS. II. Correlations between observables
- The Fundamenal Plane in CL0024 at z=0.4: Implications for the Evolution of the Mass-to-Light Ratio
- On the Origin of Cusps in Dark Matter Halos
- A Universal Density Profile for Dark and Luminous Matter?
- Luminosity Evolution of Early-type Galaxies to z=0.83: Constraints on Formation Epoch and Omega
- Global Relationships Among the Physical Properties of Stellar Systems
- Structure of Dark Matter Halos From Hierarchical Clustering
- An investigation into the prominence of spiral galaxy bulges
- WINGS: a WIde-field Nearby Galaxy-cluster Survey. I - Optical imaging
- The Tilt of the Fundamental Plane of Elliptical Galaxies: I. Dynamical and Structural Effects
- The Fundamental Plane of Gravitational Lens Galaxies and The Evolution of Early-Type Galaxies in Low Density Environments
- Weak homology of elliptical galaxies
- Galaxy merging, the Fundamental Plane of elliptical galaxies, and the Mbh-sigma relation
- Near-Infrared Imaging of Early-Type Galaxies III. The Near-Infrared Fundamental Plane
- The Fundamental Plane at z=1.27: First Calibration of the Mass Scale of Red Galaxies at Redshifts z>1
- The Tilt of the Fundamental Plane: Three-quarters Structural Nonhomology, One-quarter Stellar Population
- The Cusp/Core Problem in Galactic Halos: Long-Slit Spectra for a Large Dwarf Galaxy Sample
- The specific entropy of elliptical galaxies: an explanation for profile-shape distance indicators?
- Evolution of Early-Type Galaxies in Distant Clusters: The Fundamental Plane using HST Imaging and Keck Spectroscopy
- The structure of dark matter halos in hierarchical clustering theories
- The Evolution of Early-Type Galaxies in Distant Clusters III.: M/L_V Ratios in the z=0.33 Cluster CL1358+62
- The Inner Structure of LCDM Halos II: Halo Mass Profiles and LSB Rotation Curves
- Near-Infrared Imaging of Early-Type Galaxies IV. The Physical Origins of the Fundamental Plane Scaling Relations
- The constant density region of the dark halos of spiral galaxies
- Dependence of the Inner DM Profile on the Halo Mass
- The Properties of Field Elliptical Galaxies at Intermediate Redshift. I: Empirical Scaling Laws
- The Fundamental Plane of Ellipticals: I. The Dark Matter Connection
- Exploring Cluster Ellipticals as Cosmological Standard Rods
- The Black Hole Masses and Host Galaxies of BL Lac Objects
- The properties of field elliptical galaxies at intermediate redshift. III: the Fundamental Plane and the evolution of stellar populations from z~0.4 to z=0
- Luminosity Evolution of Field Early-Type Galaxies to z=0.55
- The Redshift Evolution of the Stellar Populations in Elliptical Galaxies
- The Mgb-sigma Relation of Elliptical Galaxies at z=0.37
- Early-type Galaxy Distances from the Fundamental Plane and Surface Brightness Fluctuations
- Galaxy clusters in the Perseus-Pisces region - II. The peculiar velocity field
- The tilt of the Fundamental Plane of Early-type galaxies: wavelength dependence
- The Near-Infrared Fundamental Plane of Elliptical Galaxies
- The Photometric Plane of Elliptical Galaxies
- On the Invariant Distribution of Galaxies in the re--mie plane out to z = 0.64
- Radial orbital anisotropy and the Fundamental Plane of elliptical galaxies
- A near infrared photometric plane for ellipticals and bulges of spirals
- Scaling relations in early-type galaxies belonging to groups
- The Fundamental Plane Evolution of Active Galactic Nucleus Host Galaxies
- Black hole masses and the Fundamental Plane of BL Lac objects
- Energy, entropy and mass scaling relations for elliptical galaxies. Towards a physical understanding of their photometric properties
- Modelling elliptical galaxies: phase-space constraints on two-component (gamma1,gamma2) models
- An Economical Technique for the Estimate of Galaxy Distances: the Photometric Fundamental Plane
- On the use of scaling relations for the Tolman test
- The scaling relations of early--type galaxies in clusters I. Surface photometry in seven nearby clusters
- Density Profile Asymptotes at the Centre of Dark Matter Halos
- The Two-Component Virial Theorem and the Physical Properties of Stellar Systems
- On Mechanics and Thermodynamics of a stellar galaxy in a two-component virial system and the Fundamental Plane
- Clausius' Virial vs. Total Potential Energy in the dynamics of a two-component system
Cited by in corpus (24)
- Central mass-to-light ratios and dark matter fractions in early-type galaxies
- The 6dF Galaxy Survey: The Near-Infrared Fundamental Plane of Early-Type Galaxies
- The SAURON project - XIII. SAURON-GALEX study of early-type galaxies: the ultraviolet colour-magnitude relations and Fundamental Planes
- On the Origin of Dwarf Elliptical Galaxies: The Fundamental Plane
- The SAURON Project - XIX. Optical and near-infrared scaling relations of nearby elliptical, lenticular and Sa galaxies
- The age dependence of the size-stellar mass relation and some implications
- Calibrating the fundamental plane with SDSS DR8 data
- SPIDER - VI. The Central Dark Matter Content of Luminous Early-Type Galaxies: Benchmark Correlations with Mass, Structural Parameters and Environment
- Secondary infall model and dark matter scaling relations in intermediate redshift early - type galaxies
- The Kormendy Relation for early-type galaxies. Dependence on the magnitude range
- The Fundamental Plane for early-type galaxies. Dependence on the magnitude range
- The Mid-Infrared Fundamental Plane of Early-Type Galaxies
- Dwarf Galaxies in the Coma Cluster: II. Spectroscopic and Photometric Fundamental Planes
- Mergers in Galaxy Groups. II. The Fundamental Plane of Elliptical Galaxies
- Minor Mergers are not enough: The importance of Major Mergers during Brightest Cluster Galaxy assembly
- The SAMI -- Fornax Dwarfs Survey II: The Stellar Mass Fundamental Plane and the Dark Matter fraction of Dwarf Galaxies
- Velocity dispersion measurements of dwarf galaxies in the Coma cluster - implications for the structure of the fundamental plane
- The Fundamental Plane in the hierarchical context
- The quantity of dark matter in early-type galaxies and its relation to the environment
- The scaling relations of galaxies back in time: the road toward virialization
- On the tilt of Fundamental Plane by Clausius' virial maximum theory
- A new framework for understanding the evolution of early-type galaxies
- A principle of corresponding states for two-component, self-gravitating fluids
- The role of dark matter in the galaxy mass-size relationship