Using the Outskirts of Galaxy Clusters to Determine Their Mass Accretion Rate

doi 10.20944/preprints201612.0057.v1
Full Text
Abstract

Available in full text

Date
Authors
Publisher

MDPI AG

Related search

Dynamical Mass Measurements of Contaminated Galaxy Clusters Using Machine Learning

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2016English

The Baryon Mass Function for Galaxy Clusters

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2006English

The Physics of Galaxy Cluster Outskirts

Space Science Reviews
AstrophysicsAstronomyPlanetary ScienceSpace
2019English

The Insignificant Evolution of the Richness-Mass Relation of Galaxy Clusters

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2014English

Hydrostatic Mass Profiles in X-Cop Galaxy Clusters

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2019English

The Mass Accretion Rate of the Young Variable Star GM Cep

Research Notes of the AAS
2018English

Cross-Correlation Weak Lensing of SDSS Galaxy Clusters III: Mass-To-Light Ratios

2007English

The Properties of Galaxies on the Outskirts of Clusters

Proceedings of the International Astronomical Union
AstrophysicsAstronomyPlanetary ScienceSpace
2004English

Comparison of the Excess Mass Around CFHTLenS Galaxy-Pairs to Predictions From a Semi-Analytic Model Using Galaxy-Galaxy-Galaxy Lensing

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2019English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2025 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy