Galaxy luminosities, stellar masses, sizes, velocity dispersions as a function of morphological type
- 1 March 2010
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 404 (4), 2087-2122
- https://doi.org/10.1111/j.1365-2966.2010.16425.x
Abstract
No abstract availableKeywords
Other Versions
This publication has 79 references indexed in Scilit:
- Evolution in the structural properties of early-type brightest cluster galaxies at small lookback time and dependence on the environmentMonthly Notices of the Royal Astronomical Society, 2009
- A search for the most massive galaxies - II. Structure, environment and formationMonthly Notices of the Royal Astronomical Society, 2008
- The σ-LCorrelation in Nearby Early-Type GalaxiesThe Astronomical Journal, 2007
- Colors, Magnitudes, and Velocity Dispersions in Early-Type Galaxies: Implications for Galaxy Ages and MetallicitiesThe Astronomical Journal, 2005
- Galaxy types in the Sloan Digital Sky Survey using supervised artificial neural networksMonthly Notices of the Royal Astronomical Society, 2004
- Quantifying the Bimodal Color‐Magnitude Distribution of GalaxiesThe Astrophysical Journal, 2004
- The Optical and Near‐Infrared Properties of Galaxies. I. Luminosity and Stellar Mass FunctionsThe Astrophysical Journal Supplement Series, 2003
- Constraints on a Universal Stellar Initial Mass Function from Ultraviolet to Near‐Infrared Galaxy Luminosity DensitiesThe Astrophysical Journal, 2003
- Early-Type Galaxies in the Sloan Digital Sky Survey. I. The SampleThe Astronomical Journal, 2003
- Stellar Mass‐to‐Light Ratios and the Tully‐Fisher RelationThe Astrophysical Journal, 2001