New Analysis of Dark Matter in Elliptical Galaxies
arXiv:2207.02945 · doi:10.1093/mnras/stac3236
Abstract
We investigate a correlation between the dark matter content of elliptical galaxies and their ellipticity that was initially reported in 2014. We use new determinations of dark matter and ellipticities that are posterior to that time. Our data set consists of 237 elliptical galaxies passing a strict set of criteria. We find a relation between the mass-to-light ratio and ellipticity that is well fit by M/L = (14.1 \pm 5.4)?, which agrees with the result reported in 2014.
References in corpus (18)
- Improving the full spectrum fitting method: accurate convolution with Gauss-Hermite functions
- The Radial Acceleration Relation in Rotationally Supported Galaxies
- Measuring the inclination and mass-to-light ratio of axisymmetric galaxies via anisotropic Jeans models of stellar kinematics
- The Sloan Lens ACS Survey. V. The Full ACS Strong-Lens Sample
- Dynamical modelling of luminous and dark matter in 17 Coma early-type galaxies
- The SL2S Galaxy-scale Lens Sample. V. Dark Matter Halos and Stellar IMF of Massive Early-type Galaxies out to Redshift 0.8
- The Sloan Lens ACS Survey. XIII. Discovery of 40 New Galaxy-Scale Strong Lenses
- MOSFIRE Spectroscopy of Quiescent Galaxies at 1.5 < z < 2.5. I - Evolution of Structural and Dynamical Properties
- The Baryon Fractions and Mass-to-Light Ratios of Early-Type Galaxies
- Systematic trends in total-mass profiles from dynamical models of early-type galaxies
- The Spectroscopy and H-band Imaging of Virgo cluster galaxies (SHIVir) Survey: Scaling Relations and the Stellar-to-Total Mass Relation
- SDSS-IV MaNGA: Internal mass distributions and orbital structures of early-type galaxies and their dependence on environment
- Detection of Enhanced Central Mass-to-Light Ratios in Low-Mass Early-Type Galaxies: Evidence for Black Holes?
- Study of gravitational fields and globular cluster systems of early-type galaxies
- A Precise Benchmark for Cluster Scaling Relations: Fundamental Plane, Mass Plane and IMF in the Coma Cluster from Dynamical Models
- Effect of gravitational field self-interaction on large structure formation
- Globular Cluster Systems and X-Ray Atmospheres in Galaxies
- Effect of the field self-interaction of General Relativity on the Cosmic Microwave Background Anisotropies