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Velocity dispersion
V. Spatially-Resolved Stellar Angular Momentum, Velocity Dispersion, and Higher Moments of the 41 Most Massive Local Early-Type Galaxies
MODEST-18: Dense Stellar Systems in the Era of Gaia, LIGO and LISA June 25 - 29, 2018 | Santorini, Greece
Astronomy 422
REDSHIFTS and VELOCITY DISPERSIONS of GALAXY CLUSTERS in the HOROLOGIUM-RETICULUM SUPERCLUSTER Matthew C
Properties of Simulated Milky Way-Mass Galaxies in Loose Group and field Environments
A 10000-Solar-Mass Black Hole in the Nucleus of a Bulgeless Dwarf Galaxy
Dark Matter in Elliptical Galaxies?
The Cosmic Distance Scale • Distance Information Is Often Crucial to Understand the Physics of Astrophysical Objects
Shapley Supercluster Survey: Mapping the filamentary Network Connecting the Clusters
The Jeans Modeling of the Milky Way Galaxy: Implications of the Kinematics of the Stellar Halo
Cosmology with Velocity Dispersion Counts: an Alternative to Measuring
Satellite Galaxy Velocity Dispersions in the SDSS and Modified Gravity Models
Arxiv:2010.00693V2 [Astro-Ph.GA] 31 Oct 2020 Total Mass of Dark Matter Around Galaxies
Arxiv:2009.11498V1 [Astro-Ph.GA] 24 Sep 2020
Stellar Evolution & Formation History of Centaurus a (NGC 5128)
Lecture G3: Galaxies: Distances
Arxiv:2011.06002V1 [Astro-Ph.CO] 11 Nov 2020
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Arxiv:2101.00013V2 [Astro-Ph.GA] 3 Aug 2021
Measurement of Black Hole Masses in Active Galactic Nuclei
Stellar Mass Versus Velocity Dispersion As Tracers of the Lensing Signal Around Bulge-Dominated Galaxies
Survey of Astrophysics A110 Galaxies
Arxiv:1808.02840V1 [Astro-Ph.GA] 8 Aug 2018 Down to an H I Mass Limit of a Few Times 10 M
The Progeny of a Cosmic Titan: a Massive Multi-Component Proto-Supercluster in Formation at Z=2.45 in VUDS⋆ O
On the Relation Between Black Hole Mass and Velocity Dispersion in Type 1 and Type 2 AGN
La Freccia Rossa
Chapter 2 Stellar Dynamics in Galaxies
Structure and Dynamics of the Shapley Supercluster
The Shapley Supercluster: the Largest Matter Concentration in the Local Universe
Predicted MOND Velocity Dispersions for a Catalog of Ultra-Diffuse Galaxies in Group Environments Oliver Müller, Benoit Famaey, Hongsheng Zhao
Supernovae-Generated High-Velocity Compact Clouds A
SDSS-IV Manga: Stellar Initial Mass Function Variation Inferred from Bayesian Analysis of the Integral field Spectroscopy of Early-Type Galaxies
Galactic Astronomy
The Cosmic Distance Ladder
On the Dependence of Spectroscopic Indices of Early-Type Galaxies on Age, Metallicity and Velocity Dispersion
Using Velocity Dispersion to Estimate Halo Mass: Is the Local Group in Tension with ΛCDM?
The GALAH Survey: Chemodynamics of the Solar Neighbourhood
Lecture 4 Clusters & Superclusters
The Milky Way and Its Components: Overview
VIII. Stellar Velocity Dispersion Profiles and Environmental Dependence of Early-Type Galaxies
The Velocity Dispersion Function of Very Massive Galaxy Clusters: Abell 2029 and Coma
The Cosmic Distance Ladder
Clusters of Galaxies
Impact of the Dark Matter Velocity Distribution on Capture Rates in The
A Measurement of the Hubble Constant from Angular Diameter Distances to Two Gravitational Lenses
Measuring Cosmological Distances Using Cluster Edges As a Standard Ruler
Dark Matter Velocity Dispersion Effects on CMB and Matter Power Spectra
Astronomy 140: Stellar Systems and Cosmology
Cosmic Distance Scale
Arxiv:1512.04661V1
THE MILKY WAY TOMOGRAPHY with SDSS. II. STELLAR METALLICITY Zˇ Eljko Ivezic´,1 Branimir Sesar,1 Mario Juric´,2 Nicholas Bond,3 Julianne Dalcanton,1 Constance M
Kinematics of Galaxies
The Milky Way's Stellar Disk
Dark Matter in Elliptical Galaxies?
Stars and Galaxies
Stellar Velocity Dispersion and Dynamical Mass of the Ultra-Diffuse
Velocity Dispersion in Elliptical Galaxies
A421 Elliptical Galaxies
The Dwarf Galaxy Population and Density Profiles
Abstract the Mond External Field Effect on Dwarf
Angular Momentum Evolution of Galaxies Over the Past 10 Gyr: a MUSE and KMOS Dynamical Survey of 400 Star-Forming Galaxies from Z = 0.3–1.7
Galaxies 626
Velocity Dispersion Around Ellipticals in MOND
Determining Stellar Velocity Dispersion in Active Galaxies: Is the [OIII] Width a Valid Surrogate?