What Are S0 Galaxies?
arXiv:0902.4718 · doi:10.1088/0004-637X/694/2/L120
Abstract
The data collected in the Shapley-Ames catalog of bright galaxies show that lenticular (S0) galaxies are typically about a magnitude fainter than both elliptical (E) and early spiral (Sa) galaxies. Hubble (1936) was therefore wrong to regard S0 galaxies as being intermediate between morphological types E and Sa. The observation that E5-E7 galaxies are significantly fainter than objects of sub-types E0-E5 suggests that many of the flattest 'ellipticals' may actually be misclassified lenticular galaxies. In particular it is tentatively suggested all E7 galaxies might actually be misclassified S0_1 (7) galaxies. The present results are consistent with the view that galaxies belonging to the S0 class evolved in environments in which they typically lost more than half of their original luminous material.
ApJ (Letters), in press; 1 postscript figure
References in corpus (1)
Cited by in corpus (20)
- A Revised Parallel-Sequence Morphological Classification of Galaxies: Structure and Formation of S0 and Spheroidal Galaxies
- A Classical Morphological Analysis of Galaxies in the Spitzer Survey of Stellar Structure in Galaxies (S4G)
- Photometric scaling relations of lenticular and spiral galaxies
- The Hubble sequence: just a vestige of merger events?
- Dissecting the Red Sequence: The Bulge and Disc Colours of Early-Type Galaxies in the Coma Cluster
- Lenticular Galaxies and Their Environments
- Ages and abundances in large-scale stellar disks of nearby S0 galaxies
- Structural and dynamical modeling of WINGS clusters. II. The orbital anisotropies of elliptical, spiral and lenticular galaxies
- The gas kinematics, excitation, and chemistry, in connection with star formation, in lenticular galaxies
- Dynamic S0 Galaxies II: the Role of Diffuse Hot Gas
- Stellar population and kinematics of NGC404
- Demographics of Isolated Galaxies Along the Hubble Sequence
- The ACS Nearby Galaxy Survey Treasury VI. The Ancient Star Forming disk of NGC 404
- Beyond Sérsic + exponential disc morphologies in the Coma Cluster
- The SMBH mass versus M_G sigma^2 relation: A comparison between real data and numerical models
- Footprints in the sand: What can globular clusters tell us about NGC 4753 past?
- The size--mass and other structural parameter () relations for local bulges/spheroids from multicomponent decompositions
- Demographics of Sloan Digital Sky Survey galaxies along the Hubble sequence
- Kinematics and Stellar Disk Modeling of Lenticular Galaxies
- Elliptical galaxies: rotationally distorted, after all