On the fundamentality of the radial acceleration relation for late-type galaxy dynamics [PDF]
Galaxies have been observed to exhibit a level of simplicity unexpected in the complex galaxy formation scenario posited by standard cosmology. This is particularly apparent in their dynamics, where scaling relations display much regularity and little ...
Richard Stiskalek, Harry Desmond
openalex +3 more sources
The SAMI galaxy survey: Mass and environment as independent drivers of galaxy dynamics [PDF]
The kinematic morphology–density relation of galaxies is normally attributed to a changing distribution of galaxy stellar masses with the local environment. However, earlier studies were largely focused on slow rotators; the dynamical properties of the
J. van de Sande +19 more
semanticscholar +1 more source
Dark Coincidences: Small-Scale Solutions with Refracted Gravity and MOND
General relativity and its Newtonian weak field limit are not sufficient to explain the observed phenomenology in the Universe, from the formation of large-scale structures to the dynamics of galaxies, with the only presence of baryonic matter.
Valentina Cesare
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Introducing the NEWHORIZON simulation: Galaxy properties with resolved internal dynamics across cosmic time [PDF]
Hydrodynamical cosmological simulations are increasing their level of realism by considering more physical processes and having greater resolution or larger statistics.
Y. Dubois +15 more
semanticscholar +1 more source
Heart of darkness: the influence of galactic dynamics on quenching star formation in galaxy spheroids [PDF]
Quenched galaxies are often observed to contain a strong bulge component. The key question is whether this reflects a causal connection – can star formation be quenched dynamically by bulges or the spheroids of early-type galaxies?
J. Gensior, J. Kruijssen, B. Keller
semanticscholar +1 more source
First Gaia dynamical model of the Milky Way disc with six phase space coordinates: a test for galaxy dynamics [PDF]
We construct the first comprehensive dynamical model for the high-quality subset of stellar kinematics of the Milky Way disc, with full 6D phase-space coordinates, provided by the Gaia Data Release 2.
M. S. Nitschai +2 more
semanticscholar +1 more source
A Fresh Look at Narrow-angle Tail Radio Galaxy Dynamics, Evolution, and Emissions [PDF]
We present a 3D magnetohydrodynamic study of narrow-angle tail (NAT) radio galaxy (RG) dynamics, including passive cosmic ray electrons. We follow the evolution of a bipolar-jet RG in a persistent crosswind through hundreds of Myr. We confirm traditional
B. O’Neill +3 more
semanticscholar +1 more source
Revealing the dynamical behavior of stars in a prolate or oblate elliptical galaxy
We consider the motion of a test particle (star) on the meridian plane (R,z) of an elliptical galaxy with an additional central nucleus component. The shape of the elliptical galaxy can be either prolate or oblate, or even spherical by simply changing ...
Eman M. Moneer +2 more
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Evidence for Galaxy Dynamics Tracing Background Cosmology Below the de Sitter Scale of Acceleration [PDF]
Galaxy dynamics probe weak gravity at accelerations below the de Sitter scale of acceleration , where c is the velocity of light and H is the Hubble parameter.
M. Putten
semanticscholar +1 more source
Self-similar galaxy dynamics below the de Sitter scale of acceleration [PDF]
Radial accelerations α in galaxy dynamics are now observed over an extended range in redshift that includes model calculations on galactic distributions of cold dark matter (CDM) in ΛCDM.
M. Putten
semanticscholar +1 more source

