Results 131 to 140 of about 51,405 (265)
Computation of bound orbits in the plane of a galaxy with a flat rotation curve [PDF]
, 2011 Michael Bacon, Amber Sharrar
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Cold gas disks in main-sequence galaxies at cosmic noon: Low turbulence, flat rotation curves, and disk-halo degeneracy [PDF]
, 2023 Federico Lelli +8 more
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Raising galaxy rotation curves via dressing
Physical Review DWe present a manifestly diffeomorphism-invariant simple model of galaxy dynamics obtained by applying the Dressing Field Method (DFM) to a general-relativistic system comprising the metric and four scalar fields, phenomenologically representing the four-velocity of a cosmological fluid or dust field.
J. François, L. Ravera
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Rotation Curve with MOND and Dark Matter Halo profile for ESO138-G014 [PDF]
, 2014 This paper is devoted to solve the galactic rotation problem for ESO138-G014 galaxy based on two theories: dark matter and Modified Newtonian Dynamics. Here we did the rotation curve analysis with two possible choices for the dark matter density profile,
Abidin, Zamri Zainal +3 more
core
Physical Parameters of Late Type Spiral Galaxies I-Mass and Luminosity of NGC 6946 [PDF]
Journal of Astronomy and Space Sciences, 1985 Using Brandt model the mass distribution of the late type spiral galaxy NGC 6946 was derived, and the total mass was reestimated to understand the M/L ratio of this galaxy. Two kinds of the rotation curve with shape parameter n = 1 and 3.3 were examined.
Sug-Whan Kim, Mun-Suk Chun
doaj
Dark Matter and Rotation Curves of Stars in Galaxies [PDF]
, 2001 Ernst Schmützer
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3D-Barolo: a new 3D algorithm to derive rotation curves of galaxies [PDF]
, 2015 Enrico M. Di Teodoro, Filippo Fraternali
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Spectroscopic Studies of Starburst Galaxies; the Dynamical Structure of Blue Compact Dwarf Galaxy Haro 6 [PDF]
Journal of Astronomy and Space Sciences, 1995 We carried out photometric and spectroscopic observations of the blue compact dwarf galaxy Haro 6 in the Virgo Cluster of Galaxies. The long-slit spectroscopy was employed at three position angles, ϕ = 0°, ϕ = 30°, and ϕ = 120° CCD camera mounted on the ...
Mun-Suk Chun +2 more
doaj
An Equilibrium Model of the Galaxy Determined by Element Abundance Gradients
The Astrophysical JournalWe present a method to determine the gravitational potential of the Milky Way from measurements of the locations, velocities, and element abundances of stars in the Galactic disk.
Lawrence M. Widrow +4 more
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