Results 1 to 10 of about 787 (130)

Kinematics, substructure and luminosity-weighted dynamics of six nearby galaxy groups [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2006
15 pages, 5 figures. Accepted for publication in MNRAS.
Firth, P.   +5 more
openaire   +5 more sources

Kinematics and dynamics of the luminous infrared galaxy pair NGC 5257/58 (Arp 240) [PDF]

open access: yesAstronomy & Astrophysics, 2018
Context. Encounters between galaxies modify their morphology, kinematics, and star formation history. The relation between these changes and external perturbations is not straightforward. The great number of parameters involved requires both the study of large samples and individual encounters where particular ...
Fuentes-Carrera, I.   +8 more
openaire   +7 more sources

The SAMI Galaxy Survey: Kinematics of Stars and Gas in Brightest Group Galaxies—The Role of Group Dynamics [PDF]

open access: yesThe Astrophysical Journal, 2021
Abstract We study the stellar and gas kinematics of the brightest group galaxies (BGGs) in dynamically relaxed and unrelaxed galaxy groups for a sample of 154 galaxies in the SAMI galaxy survey. We characterize the dynamical state of the groups using the luminosity gap between the two most luminous galaxies and the BGG offset from the ...
Mojtaba Raouf   +19 more
openaire   +2 more sources

Evaluating galaxy dynamical masses from kinematics and jeans equilibrium in simulations [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2021
ABSTRACT We provide prescriptions to evaluate the dynamical mass (Mdyn) of galaxies from kinematic measurements of stars or gas using analytic considerations and the VELA suite of cosmological zoom-in simulations at z = 1–5. We find that Jeans or hydrostatic equilibrium is approximately valid for galaxies of stellar masses above M⋆ ∼ 109.
Michael Kretschmer   +5 more
openaire   +2 more sources

Kinematics and dynamics of the haloes of supergiant galaxies [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 1985
On presente des mesures de la cinematique interne des halos de 3 galaxies supergeantes dans des amas moderement riches. On trouve que les profils de la dispersion des vitesses sont plats ou croissent avec le rayon.
D. Carter   +4 more
openaire   +1 more source

Kinematical and Dynamical Modeling of Elliptical Galaxies [PDF]

open access: yesEAS Publications Series, 2006
Elements of kinematical and dynamical modeling of elliptical galaxies (Es) are presented. In projection, NFW models resemble Sersic models, but with a very narrow range of shapes (m=3+/-1). The total density profile of Es cannot be NFW-like because the predicted local M/L and aperture velocity dispersion within an effective radius (Re) are much lower ...
Mamon, G. A.   +4 more
openaire   +2 more sources

Kinematics and dynamics of the "superthin" edge-on disk galaxy IC 5249 [PDF]

open access: yesAstronomy & Astrophysics, 2001
11 pages and 8 figures. Accepted for Astronomy and Astrophysics (September 2001)
van der Kruit, P C   +3 more
openaire   +2 more sources

Photometry, Kinematics and Dynamics of the Barred Galaxy NGC 5383 [PDF]

open access: yesSymposium - International Astronomical Union, 1983
NGC 5383 has often been used as a prototype of SB(s)b type galaxies, particulary in studies of gas flow. We have therefore set out to complement the existing data with surface photometry, velocity measurements in the bar and a dynamical model.
E. Athanassoula, M. F. Duval
openaire   +1 more source

Structure and kinematics of edge-on galaxy discs - V. The dynamics of stellar discs [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2005
Accepted for publication by Mon. Not.
Kregel, M   +2 more
openaire   +5 more sources

Made-to-measure dynamical particle models of elliptical galaxies [PDF]

open access: yes, 2007
NMAGIC modelling: Syer and Tremaine (1996) proposed a made-to-measure (M2M) algorithmto construct N-particle systems from observational data and used it to generate a triaxial model from density observables.
De Lorenzi, F., De Lorenzi, Flavio
core   +1 more source

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