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相关论文: Mass-Diameter Relation of Globular Star Clusters, …

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In this work we determine the total globular cluster (GC) counts and globular cluster system (GCS) total mass estimates for 27 extremely massive elliptical galaxies. The GC 2D spatial distributions of these galaxies were created from…

星系天体物理 · 物理学 2025-07-16 Veronika Dornan , William E. Harris

The formation of compact objects like stars and black holes is strongly constrained by the requirement that nearly all of the initial angular momentum of the diffuse material from which they form must be removed or redistributed during the…

太阳与恒星天体物理 · 物理学 2010-01-06 Richard B. Larson

I will argue that the inertial mass is greater than the gravitational mass for all objects which are held together primarily by gravitational forces. Thus, for celestial objects, like planets, stars and galaxies, their inertial mass is…

综合物理 · 物理学 2016-03-08 Gregory W. Horndeski

We consider the hypothesis that the formation of elliptical galaxies includes a phase in which star formation is mostly restricted to massive stars, with the bias towards high mass stars increasing with elliptical galaxy mass. The mass…

天体物理学 · 物理学 2009-10-28 Stephen E. Zepf , Joseph Silk

In the past years a wealth of observations has allowed us to unravel the structural properties of the Dark and Luminous mass distribution in spirals. As result, it has been found that their rotation curves follow, out their virial radius,…

天体物理学 · 物理学 2009-11-13 Paolo Salucci

The discovery of acceleration of the universe expansion in recent astrophysics research prompts the author to propose that the Newton's gravitation law can be generalized to accommodate the antimatter: While the force between…

综合物理 · 物理学 2007-05-23 Guang-Jiong Ni

Gravitation is the common underlying texture between General Relativity and Quantum Mechanics. We take gravitation as the link that can make possible the marriage between these two sciences. We use here the duality of Nature for…

综合物理 · 物理学 2008-11-26 Antonio Alfonso-Faus

By numerically solving the mass distribution in a rotating disk based on Newton's laws of motion and gravitation, we demonstrate that the observed flat rotation curves for most spiral galaxies correspond to exponentially decreasing mass…

星系天体物理 · 物理学 2011-08-17 James Q. Feng , C. F. Gallo

The evidence of the phenomenon for which, in galaxies, the gravitating mass is distributed differently than the luminous mass, increases as new data become available. Furthermore, this discrepancy is well structured and it depends on the…

星系天体物理 · 物理学 2019-03-11 Paolo Salucci

We discuss the circumstances under which gravity might be repulsive rather than attractive. In particular we show why our standard solar system distance scale gravitational intuition need not be a reliable guide to the behavior of…

广义相对论与量子宇宙学 · 物理学 2022-10-12 Philip D. Mannheim

No experiment to date has provided evidence for quantum features of the gravitational interaction. Recently proposed tests suggest looking for the generation of quantum entanglement between massive objects as a possible route towards the…

量子物理 · 物理学 2020-01-31 Tanjung Krisnanda , Guo Yao Tham , Mauro Paternostro , Tomasz Paterek

Elliptical galaxies formed in a major merger tend to become more nearly spherical with time, thanks to the gravitational effect of their central black hole (or black holes). Observational results indicate that elliptical galaxies with older…

天体物理学 · 物理学 2017-08-23 Barbara Ryden , Jeremy Tinker

Traditionally globular clusters and dwarf spheroidal galaxies have been distinguished by using one or more of the following criteria: (1) mass, (2) luminosity, (3) size, (4) mass-to-light ratio and (5) spread in metallicity. However, a few…

天体物理学 · 物理学 2009-11-13 Sidney van den Bergh

We explore the mass distribution of material associated with galaxies from the observation of gravitational weak lensing for the galaxy mass correlation function with the aid of $N$-body simulations of dark matter. The latter is employed to…

宇宙学与河外天体物理 · 物理学 2015-05-28 Shogo Masaki , Masataka Fukugita , Naoki Yoshida

Elliptical galaxies have been observed to cluster near a ribbon along a two-dimensional plane (the Fundamental Plane of Elliptical Galaxies) in the three dimensional space of effective radius, effective surface brightness and central…

天体物理学 · 物理学 2016-08-30 S. E. Levine

In this article, we examine a model which proposes a common explanation for the presence of additional attractive gravitational effects -- generally considered to be due to dark matter -- in galaxies and in clusters, and for the presence of…

天体物理学 · 物理学 2007-05-23 Alexandre Arbey

We construct a multimetric gravity theory containing N >= 3 copies of standard model matter and a corresponding number of metrics. In the Newtonian limit, this theory generates attractive gravitational forces within each matter sector, and…

广义相对论与量子宇宙学 · 物理学 2010-07-07 Manuel Hohmann , Mattias N. R. Wohlfarth

In the present work we derive an analytical expression for the mass density of an object with spherical symmetry, whose corresponding potential allows obtaining a circular velocity around it that is in agreement with the observed rotation…

星系天体物理 · 物理学 2023-02-09 José Enrique Hernández Ramírez

The total mass M_GCS in the globular cluster (GC) system of a galaxy is empirically a near-constant fraction of the total mass M_h = M_bary + M_dark of the galaxy, across a range of 10^5 in galaxy mass. This trend is radically unlike the…

星系天体物理 · 物理学 2017-02-15 William E. Harris , John P. Blakeslee , Gretchen L. H. Harris

The mass-size relation is a fundamental galaxy scaling law closely tied to galaxy formation and evolution. Using added-value products of the Calar Alto Void Integral-field Treasury surveY (CAVITY) and SDSS DR16 images, we examine the effect…