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相关论文: Tully-Fisher Relations and Retardation Theory for …

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Galaxies are huge physical systems having dimensions of many tens of thousands of light years. Thus any change at the galactic center will be noticed at the rim only tens of thousands of years later. Those retardation effects seems to be…

综合物理 · 物理学 2025-05-27 Asher Yahalom

Galaxies are gigantic physical systems having a typical size of many tens of thousands of light years. Thus any change at the center of the galaxy will affect the rim only tens of millennia later. Those retardation effects seems to be…

综合物理 · 物理学 2021-08-21 Asher Yahalom

We argue that soft gravitational radiation leads to a misidentification of the angular momentum of stars seen in distant galaxies, and that this could be interpreted as an additional mass inside the orbit of the star. It is tempting to…

高能物理 - 理论 · 物理学 2018-10-16 Tom Banks , Willy Fischler

We explore the Tully-Fisher relation over five decades in stellar mass in galaxies with circular velocities ranging over 30 < Vc < 300 km/s. We find a clear break in the optical Tully-Fisher relation: field galaxies with Vc < 90 km/s fall…

天体物理学 · 物理学 2009-10-31 Stacy McGaugh , Jim Schombert , Greg Bothun , Erwin de Blok

We have studied the origin of the Tully-Fisher relation by analysing hydrodynamical simulations in a Lambda-CDM universe. We found that smaller galaxies exhibit lower stellar masses than those predicted by the linear fit to high mass…

宇宙学与河外天体物理 · 物理学 2011-01-13 Maria E. De Rossi , Patricia B. Tissera , Susana E. Pedrosa

The rotation curves of spiral galaxies obey strong scaling relations. These include the Tully-Fisher and baryonic Tully-Fisher relations, and the mass discrepancy--acceleration relation. These relations can be used to place constraints on…

天体物理学 · 物理学 2009-11-11 Stacy McGaugh

We study the location of massive disk galaxies on the Tully-Fisher relation. Using a combination of K-band photometry and high-quality rotation curves, we show that in traditional formulations of the TF relation (using the width of the…

天体物理学 · 物理学 2009-11-13 E. Noordermeer , M. A. W. Verheijen

The Tully-Fisher Relation (TFR) links two fundamental properties of disk galaxies: their luminosity and their rotation velocity (mass). The pioneering work of Vogt et al. in the 1990's showed that it is possible to study the TFR for spiral…

天体物理学 · 物理学 2015-06-24 Alfonso Aragon-Salamanca

We find a new Tully-Fisher-like relation for spiral galaxies holding at different galactocentric radii. This Radial Tully-Fisher (RTF) relation allows us to investigate the distribution of matter in the optical regions of spiral galaxies.…

天体物理学 · 物理学 2008-11-26 Irina A. Yegorova , Paolo Salucci

The redshift evolution of the Tully-Fisher Relation probes gravitational dynamics that must be consistent with any modified gravity theory seeking to explain the galactic rotation curves without the need for dark matter. Within the context…

天体物理学 · 物理学 2008-09-18 Christopher Limbach , Dimitrios Psaltis , Feryal Ozel

We present a study of the stellar and baryonic Tully-Fisher relation within the redshift range of $0.6 \leq z \leq 2.5$ utilizing observations of \sfgs. This dataset, as explored in \citet{GS23}, comprises of disk-like galaxies spanning a…

星系天体物理 · 物理学 2024-09-25 Gauri Sharma , Varenya Upadhyaya , Paolo Salucci , Shantanu Desai

Rotation curves of spiral galaxies \emph{i}) fall off much less steeply than the Keplerian curves do, and \emph{ii}) have asymptotic speeds almost proportional to the fourth root of the mass of the galaxy, the Tully-Fisher relation. These…

广义相对论与量子宇宙学 · 物理学 2010-11-02 Y. Sobouti , A. Hasani Zonoozi , H. Haghi

We use optical rotation curves to investigate the R-band Tully-Fisher properties of a sample of 90 spiral galaxies in close pairs. The galaxies follow the Tully-Fisher relation remarkably well, with the exception of eight distinct 3-sigma…

The observed radial velocity of a galaxy consists of two main components: the recession velocity caused by the smooth Hubble expansion and the peculiar velocity resulting from the gravitational attraction of growing structures due to matter…

宇宙学与河外天体物理 · 物理学 2023-10-25 Khaled Said

Galaxies and galaxy clusters have rotational velocities apparently too fast to allow them to be gravitationally bound by their visible matter. This has been attributed to the presence of invisible (dark) matter, but so far this has not been…

综合物理 · 物理学 2015-06-05 M. E. McCulloch

There is a large observational scatter toward low velocities in the stellar mass Tully-Fisher relation if disturbed and compact objects are included. However, this scatter can be eliminated if one replaces rotation velocity with $\rm S_{\rm…

星系天体物理 · 物理学 2010-01-22 M. D. Covington , S. A. Kassin , A. A. Dutton , B. J. Weiner , T. J. Cox , P. Jonsson , J. R. Primack , S. M. Faber , D. C. Koo

Modifications to Newtonian dynamics at low accelerations have long been proposed as an alternative to dark matter to explain galaxy rotation curves. More recently, similar corrections have been invoked to interpret anomalies in…

星系天体物理 · 物理学 2026-03-19 Riccardo Scarpa , Renato Falomo , Aldo Treves

We predict the Tully-Fisher (TF) and surface-brightness--magnitude relation for disk galaxies at z=3 and discuss the origin of these scaling relations and their scatter. We show that the variation of the TF relation with redshift can be a…

天体物理学 · 物理学 2016-08-30 Ari Buchalter , Raul Jimenez , Marc Kamionkowski

In any physical system, when we move from short to large scales, new spacetime symmetries emerge which help us to simplify the dynamics of the system. In this letter we demonstrate that certain variations on the symmetries of General…

广义相对论与量子宇宙学 · 物理学 2023-11-13 Ivan Arraut

We measure the relation between galaxy luminosity and disk circular velocity (the Tully-Fisher [TF] relation), in the g, r, i, and z-bands, for a broadly selected sample of galaxies from the Sloan Digital Sky Survey, with the goal of…

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