Results 21 to 30 of about 116,947 (262)
SMOOTHING ROTATION CURVES AND MASS PROFILES [PDF]
The Astrophysical Journal, 2015 Minor corrections in proofs and updates to references, 16 pages, 16 ...
Berrier, Joel C., Sellwood, J. A.
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Galaxies, 2018 Spiral galaxies are spinning, internally densified objects. The Virial Theorem explains galactic rotation curves via its linkage of the rotation rate to the gravitational self-potential (Ug) and the moment of inertia of oblate spheroids.
Robert E. Criss, Anne M. Hofmeister
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Rotation Curves of High-Luminosity Spiral Galaxies and the Rotation Curve of our Galaxy [PDF]
Symposium - International Astronomical Union, 1979 Rotation curves of high luminosity spiral galaxies are flat, to distances as great as r=49 kpc. This implies a significant mass at large r. Rotational velocities increase about 20 km/s across a spiral arm, as predicted by the density wave theory. By analogy, it is suggested that our Galaxy has a flat rotation curve out to r∼60 kpc, with V ∼ constant at
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Galaxy Rotation Curves in Covariant Hořava-Lifshitz Gravity
Galaxies, 2013 Using the multiplicity of solutions for the projectable case of the covariant extension of Hořava-Lifshitz gravity, we show that an appropriate choice for the auxiliary field allows for an effective description of galaxy rotation curves. This description
Jean Alexandre, Martyna Kostacinska
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Global Spine Journal, 2022 Study Design: Retrospective cross-sectional study. Objectives: It is generally believed that the apical vertebra has the largest axial rotation in adolescent idiopathic scoliosis.
Kristóf József MD +6 more
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The peculiar rotation curve of NGC 157 [PDF]
Monthly Notices of the Royal Astronomical Society, 1998 26 pages, 15 figures, LaTeX, uses mn-1.4.sty.
Ryder, S. D. +4 more
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Relativistic corrections to the rotation curves of disk galaxies
European Physical Journal C: Particles and Fields, 2021 We present a method to investigate relativistic effects arising from large masses. The method is non-perturbative and employs a mean-field approximation and gravitational lensing.
Alexandre Deur
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Numerical analysis of galactic rotation curves [PDF]
Astrophysics and Space Science, 2015 In this paper we present the discussion on the salient points of the computational analysis that are at the basis of the paper \emph{Rotation Curves of Galaxies by Fourth Order Gravity} \citep{StSc}. In fact in this paper any galactic component (bulge, disk and Dark matter component) required an onerous numerical computation since the Gauss theorem is ...
Scelza, G., Stabile, A.
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Modeling the Rising Tails of Galaxy Rotation Curves
Galaxies, 2019 It is well known, but under-appreciated in astrophysical applications, that it is possible for gravity to take on a life of its own in the form of Weyl-curvature-only metrics (note that we are referring to the Weyl-only solutions of ordinary General ...
Fan Zhang
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The universal rotation curve of spiral galaxies [PDF]
Monthly Notices of the Royal Astronomical Society: Letters, 2006 Abstract The observed strong dark-to-luminous matter coupling is described by a bias relation between visible and dark matter sources. We discuss the bias which emerges in the case where the topological structure of the Universe at very large distances does not properly match that of the Friedman space. With the use of such ‘topological’
Kirillov, AA, Turaev, D
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