Results 11 to 20 of about 106,851 (294)

Uncertainties in galaxy rotation curves [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2021
Assessing the likelihood that the rotation curve of a galaxy matches predictions from galaxy formation simulations requires that the uncertainties in the circular speed as a function of radius derived from the observational data be statistically robust ...
J. Sellwood, K. Spekkens, Carter Eckel
semanticscholar   +4 more sources

The Mass Distribution and Rotation Curve in the Galaxy [PDF]

open access: yes, 2013
The mass distribution in the Galaxy is determined by dynamical and photometric methods. The dynamical method is based on the Virial theorem, and calculates the mass from kinematical data such as rotation velocities, velocity dispersions, and motions of ...
Y. Sofue
semanticscholar   +4 more sources

The Discrepancy in Galaxy Rotation Curves

open access: yes, 2019
In this work we try a new approach for dealing with the discrepancy between observed galaxy rotation curves and theoretical predictions. This new approach does not involve any changes in the current fundamental laws of nature or the addition of dark ...
R. Gomel, Tomer Zimmerman
semanticscholar   +3 more sources

The unexpected diversity of dwarf galaxy rotation curves [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2015
We examine the circular velocity profiles of galaxies in A cold dark matter (CDM) cosmological hydrodynamical simulations from the EAGLE and LOCAL GROUPS projects and compare them with a compilation of observed rotation curves of galaxies spanning a wide
K. Oman   +11 more
semanticscholar   +9 more sources

The Survival of the Sagittarius Dwarf Galaxy and the Flatnessof the Rotation Curve of the Galaxy [PDF]

open access: yesThe Astrophysical Journal, 1998
How has the "fluffy" Sgr dwarf galaxy survived its 10-20 pericentric passages in the halo of the Milky Way for a Hubble time? The scenario that Sgr was deflected to its current orbit by the Magellanic Clouds after a rendezvous on the north Galactic pole ...
HongSheng Zhao
semanticscholar   +3 more sources

THE ASYMMETRIC DRIFT AND THE ROTATION CURVE OF THE GALAXY

open access: yesOdessa Astronomical Publications, 2014
Asymmetric drift in the solar neighbourhood is studied by the means of the RAVE data. The asymmetric drift correction is applied to the SDSS data to measure the rotation curve of the Milky Way in the extended solar neighbourhood.
O. Golubov
doaj   +2 more sources

Galaxy rotation curves in the Grumiller's modified gravity [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2012
The effective potential in the Grumiller's modified gravity includes the Newtonian potential and a Rindler term. The fitting to the rotation curve data of eight galaxies suggests a universal Rindler acceleration a approximate to 0.30 x 10(-10) ms(-2). We
Hai-Nan Lin   +3 more
semanticscholar   +4 more sources

The Rotation Curves of Galaxies [PDF]

open access: bronzeSymposium - International Astronomical Union, 1975
Currently available data on rotation curves are reviewed. For curves derived from optical measurements the distribution of the ratios: the last measured point on a rotation curve to the optical radius of the galaxy has a median value of if Reference Catalogue radii are used and if Holmberg radii are used.
M. S. Roberts
openalex   +3 more sources

Dark Matter and Rotation Curves of Stars in Galaxies [PDF]

open access: greenAstronomische Nachrichten, 2001
The dark matter accretion theory (around a central body) of the author on the basis of his 5-dimensional Projective Unified Field Theory (PUFT) is applied to the orbital motion of stars around the center of the Galaxy. The departure of the motion from Newtonian mechanics leads to approximately flat rotation curves being in rough accordance with the ...
Ernst Schmützer
openalex   +6 more sources

Detection of the Keplerian decline in the Milky Way rotation curve [PDF]

open access: yesAstronomy & Astrophysics, 2023
Our position inside the Galactic disc had prevented us from establishing an accurate rotation curve, until the advent of Gaia, whose third data release (Gaia DR3) made it possible to specify it up to twice the optical radius.
Y. Jiao   +6 more
semanticscholar   +1 more source

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