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Mass-to-Light Ratios of Early- and Late-Type Galaxies
Published online by Cambridge University Press: 26 May 2016
Abstract
Using the 100k data release of the 2dF Galaxy Redshift Survey (2dFGRS), we obtain mass-to-light ratios for isolated “host” galaxies via the dynamics of satellite galaxies which orbit about them. Distinct differences are seen in the dependence of M/L on host luminosity for early-type vs. late-type hosts.
- Type
- Part 4: Lensing
- Information
- Symposium - International Astronomical Union , Volume 220: Dark Matter in Galaxies , 2004 , pp. 145 - 146
- Copyright
- Copyright © Astronomical Society of the Pacific 2004