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相关论文: Dynamical modelling of luminous and dark matter in…

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This article describes the Schwarzschild orbit superposition method. It is the state-of-the-art dynamical modelling tool for early-type galaxies. Tests with analytic models show that masses and orbital anisotropies of not too face-on…

宇宙学与河外天体物理 · 物理学 2015-06-11 Jens Thomas

Axisymmetric, orbit-based dynamical models are used to derive dark matter scaling relations for Coma early-type galaxies. From faint to bright galaxies halo core-radii and asymptotic circular velocities increase. Compared to spirals of the…

天体物理学 · 物理学 2011-02-11 J. Thomas , R. P. Saglia , R. Bender , D. Thomas , K. Gebhardt , J. Magorrian , E. M. Corsini , G. Wegner

We studied the stellar populations, distribution of dark matter, and dynamical structure of a sample of 25 early-type galaxies in the Coma and Abell 262 clusters. We derived dynamical mass-to-light ratios and dark matter densities from…

宇宙学与河外天体物理 · 物理学 2015-06-12 E. M. Corsini , G. A. Wegner , J. Thomas , R. P. Saglia , R. Bender , S. B. Pu

We use oblate axisymmetric dynamical models including dark halos to determine the orbital structure of intermediate mass to massive Coma early-type galaxies. We find a large variety of orbital compositions. Averaged over all sample galaxies…

(Shortened) The combination of lensing and stellar dynamics breaks the mass-anisotropy degeneracy and provides stringent constraints on the mass distribution in early-type (E/S0) galaxies out to z~1. We present the combined results from the…

天体物理学 · 物理学 2009-11-10 Tommaso Treu , Leon V. E. Koopmans

Dynamical properties of two-component galaxy models whose stellar density distribution is described by a gamma-model while the total density distribution has a pure r^(-2) profile, are presented. The orbital structure of the stellar…

天体物理学 · 物理学 2009-11-13 Luca Ciotti , Lucia Morganti , Tim de Zeeuw

(Abridged) We present mass models of a sample of 14 spiral and 14 S0 galaxies that constrain their stellar and dark matter content. For each galaxy we derive the stellar mass distribution from near-infrared photometry under the assumptions…

星系天体物理 · 物理学 2011-04-07 Michael J. Williams , Martin Bureau , Michele Cappellari

Mass models of 15 nearby dwarf and spiral galaxies are presented. The galaxies are selected to be homogeneous in terms of the method used to determine their distances, the sampling of their rotation curves (RCs) and the mass-to-light ratio…

星系天体物理 · 物理学 2015-06-18 Toky Randriamampandry , Claude Carignan

We present the results of a study of the average mass profile around galaxies using weak gravitational lensing. We use 45.5 deg^2 of R_C band imaging data from the Red-Sequence Cluster Survey (RCS) and define a sample of 1.2\times 10^5…

天体物理学 · 物理学 2007-05-23 Henk Hoekstra , Howard K. C. Yee , Michael D. Gladders

Dynamical models are used to study dark matter (DM) in galaxies, how galaxies assemble through mergers, and to test galaxy formation models. Despite its widespread use, there has been no systematic study quantifying how much information can…

星系天体物理 · 物理学 2025-11-14 Paula Gherghinescu , Eugene Vasiliev , Payel Das , Justin Read

We present radially resolved spectroscopy of 8 early-type galaxies in Abell~262, measuring rotation, velocity dispersion, $H_3$ and $H_4$ coefficients along three axes, and line-strength index profiles of Mg, Fe and H$\beta$. Ionized-gas…

宇宙学与河外天体物理 · 物理学 2015-06-05 G. A. Wegner , E. M. Corsini , J. Thomas , R. P. Saglia , R. Bender , S. B. Pu

An axially symmetric galactic gravitational model composed of a dense, massive and spherical nucleus with an additional dark matter halo component was used, to distinguish between the regular and chaotic character of orbits of stars that…

星系天体物理 · 物理学 2017-09-28 Euaggelos E. Zotos , Nicolaos D. Caranicolas

The kinematics of stars and planetary nebulae in early type galaxies provide vital clues to the enigmatic physics of their dark matter halos. We fit published data for fourteen such galaxies using a spherical, self-gravitating model with…

宇宙学与河外天体物理 · 物理学 2015-05-18 Curtis J. Saxton , Ignacio Ferreras

We study the dark and luminous mass distributions, circular velocity curves (CVC), line-of-sight kinematics, and angular momenta for a sample of 42 cosmological zoom simulations of massive galaxies. Using a temporal smoothing technique, we…

宇宙学与河外天体物理 · 物理学 2014-04-02 Xufen Wu , Ortwin Gerhard , Thorsten Naab , Ludwig Oser , Inma Martinez-Valpuesta , Michael Hilz , Eugene Churazov , Natalya Lyskova

We present first results of a program to study the dynamics of undisturbed bulgeless, low surface density disk galaxies in order to probe the underlying structure of dark matter halos. High resolution H-alpha rotation curves are combined…

天体物理学 · 物理学 2007-05-23 J. J. Dalcanton , R. A. Bernstein

We investigate the well-known correlations between the dynamical mass-to-light ratio M/L and other global observables of elliptical (E) and lenticular (S0) galaxies. We construct two-integral Jeans and three-integral Schwarzschild dynamical…

[Abridged] We analyse the dark matter (DM) halo properties of 127 0.3<z<1.5 star-forming galaxies (SFGs) down to low stellar masses (8<log(Mstar/Msun)<11), using data from the MUSE Hubble Ultra Deep Field Survey and photometry from HST and…

星系天体物理 · 物理学 2026-04-01 B. I. Ciocan , N. F. Bouché , J. Fensch , W. Mercier , D. Krajnović , J. Richard , T. Contini , A. Jeanneau

We present new constraints on the density profiles of dark matter (DM) halos in seven nearby dwarf galaxies from measurements of their integrated stellar light and gas kinematics. The gas kinematics of low mass galaxies frequently suggest…

Gravitational lensing and stellar dynamics provide two complementary, nearly orthogonal, constraints on the mass distribution of early-type lens galaxies. This allows the luminous and dark-matter distribution in higher-redshift (z>0.1)…

天体物理学 · 物理学 2007-05-23 L. V. E. Koopmans

We present models for the dark and luminous mass structure of 12 strong lensing early-type galaxies (ETGs). We combine pixel-based modelling of multiband HST/ACS imaging with Jeans modelling of kinematics obtained from Keck/ESI spectra to…

星系天体物理 · 物理学 2018-02-06 Lindsay Oldham , Matthew Auger
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