How non-linear scaling relations unify dwarf and giant elliptical galaxies
arXiv:1009.5002 · doi:10.1051/eas/1148052
Abstract
Dwarf elliptical galaxies are frequently excluded from bright galaxy samples because they do not follow the same linear relations in diagrams involving effective half light radii R_e or mean effective surface brightnesses <mu>_e. However, using two linear relations which unite dwarf and bright elliptical galaxies we explain how these lead to curved relations when one introduces either the half light radius or the associated surface brightness. In particular, the curved <mu>_e - R_e relation is derived here. This and other previously misunderstood curved relations, once heralded as evidence for a discontinuity between faint and bright elliptical galaxies at M_B ~ -18 mag, actually support the unification of such galaxies as a single population whose structure (i.e. stellar concentration) varies continuously with stellar luminosity and mass.
4 pages including 2 figures, to appear in "A Universe of dwarf galaxies", Conf. Proc. (Lyon, June 14-18, 2010)
References in corpus (12)
- Star Formation Histories, Abundances and Kinematics of Dwarf Galaxies in the Local Group
- The SAURON project -- IX. A kinematic classification for early-type galaxies
- Structural Properties of Pseudo-Bulges, Classical Bulges and Elliptical Galaxies: an SDSS Perspective
- An expanded M_bh-sigma diagram, and a new calibration of active galactic nuclei masses
- Quantifying the Coexistence of Massive Black Holes and Dense Nuclear Star Clusters
- The SAURON project - XII. Kinematic substructures in early-type galaxies: evidence for disks in fast rotators
- Bulges Of Nearby Galaxies With Spitzer: Scaling Relations in Pseudobulges and Classical Bulges
- Black Holes in Pseudobulges and Spheroidals: A Change in the Black Hole-Bulge Scaling Relations at Low Mass
- The ACS Fornax Cluster Survey. II. The Central Brightness Profiles of Early-Type Galaxies: A Characteristic Radius on Nuclear Scales and the Transition from Central Luminosity Deficit to Excess
- Curvature in the color-magnitude relation but not in color-sigma: Major dry mergers at M* > 2 x 10^11 Msun?
- On the origin of the scatter around the Fundamental Plane: correlations with stellar population parameters
- The effect of dry mergers on the color-magnitude relation of early-type galaxies
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- The (black hole mass)-(host spheroid luminosity) relation at high and low masses, the quadratic growth of black holes, and intermediate-mass black hole candidates
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- Stellar populations of classical and pseudo-bulges for a sample of isolated spiral galaxies
- The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship
- Mirages in galaxy scaling relations
- A new fitting concept for the robust determination of Sérsic model parameters
- Past, present and Future of the Scaling Relations of Galaxies and Active Galactic Nuclei