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相关论文: A Theory of Changes and the Fundamental Plane

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In this paper we explore several structural and dynamical effects on the projected velocity dispersion as possible causes of the fundamental plane (FP) tilt of elliptical galaxies. Specifically, we determine the size of the systematic trend…

天体物理学 · 物理学 2015-06-24 L. Ciotti , B. Lanzoni , A. Renzini

The Fundamental Plane (FP) is an empirical relation between the size, surface brightness, and velocity dispersion of early-type galaxies. This relation has been studied extensively for early-type galaxies in the local universe to constrain…

宇宙学与河外天体物理 · 物理学 2015-06-17 Rachel Bezanson , Pieter G. van Dokkum , Jesse van de Sande , Marijn Franx , Joel Leja , Mariska Kriek

We have used the ESO Nearby Abell Cluster Survey (ENACS) in combination with the Cosmos Galaxy Catalogue, to investigate the existence of a Fundamental Plane (FP) for rich clusters of galaxies. The 20 clusters with the most regular…

天体物理学 · 物理学 2007-05-23 C. Adami , A. Mazure , A. Biviano , P. Katgert , G. Rhee

Observations consistently show that elliptical galaxies follow a tight "fundamental plane" scaling relation between size, mean surface brightness and velocity dispersion, with the form $R \propto \sigma^{a}\mu^{b}$. This relation not only…

星系天体物理 · 物理学 2015-06-19 Dan S. Taranu , John Dubinski , H. K. C. Yee

The global properties of elliptical galaxies are connected through the so-called fundamental plane of ellipticals, which is an empirical relation between their parameters: effective radius, central velocity dispersion and mean surface…

星系天体物理 · 物理学 2018-12-31 Vesna Borka Jovanović , Predrag Jovanović , Duško Borka , Salvatore Capozziello

Studies of the Fundamental Plane of early-type galaxies, from small to intermediate redshifts, are often carried out under the guiding principle that the Fundamental Plane reflects the existence of an underlying mass-luminosity relation for…

天体物理学 · 物理学 2015-06-24 Giuseppe Bertin

This article reviews the popular reasons for the belief that dwarf elliptical galaxies and (ordinary) elliptical galaxies are distinct and separate species. They include: light-profile shape (or similarly image concentration); the…

天体物理学 · 物理学 2012-04-26 Alister W. Graham

Context. The Fundamental Plane (FP) relation and the distribution of early-type galaxies (ETGs) in the FP projections, cannot be easily explained in the hierarchical framework, where galaxies grow up by merging and star formation episodes.…

星系天体物理 · 物理学 2022-06-01 Mauro D'Onofrio , Cesare Chiosi

Context: Using the Illustris-1 and IllustrisTNG-100 simulations we investigate the properties of the Fundamental Plane (FP), that is the correlation between the effective radius Re, the effective surface intensity Ie and the central stellar…

星系天体物理 · 物理学 2024-04-25 Mauro D'Onofrio , Cesare Chiosi

Early-type dwarf galaxies are the most common type of galaxies observed in the Universe. The origin of this kind of systems is still not well understood. The aim of this paper is to investigate whether the different locations of dwarf…

天体物理学 · 物理学 2009-11-13 J. A. L. Aguerri , C. Gonzalez-Garcia

We have developed an effective simulation method and applied it to the problem of the accretion of very dense secondary companions by tenuous primaries. We have studied the accretion of objects of varying luminosity ratios, with sizes and…

天体物理学 · 物理学 2009-10-31 Kelly Holley-Bockelmann , Douglas O. Richstone

In the context of modified Newtonian dynamics, the fundamental plane, as the observational signature of the Newtonian virial theorem, is defined by high surface brightness objects that deviate from being purely isothermal: the line-of-sight…

宇宙学与河外天体物理 · 物理学 2015-05-18 R. H. Sanders

We perform numerical simulations of galaxy mergers between star-forming and gas-rich spirals in order to explore the origin of the Fundamental Plane (FP) of elliptical galaxies. We consider particularly that the origin of the slope of the…

天体物理学 · 物理学 2009-10-30 Kenji Bekki

Properties of groups of galaxies depend sensitively on the algorithm for group selection, and even the most recent catalogs of groups built from redshift-space selection should suffer from projections and infalling galaxies. The…

天体物理学 · 物理学 2015-06-24 Gary A. Mamon

We present measurements of the Fundamental Plane (FP) parameters (the effective radius, the mean effective surface brightness, and the central velocity dispersion) of six field elliptical galaxies at intermediate redshift. The imaging is…

天体物理学 · 物理学 2010-04-21 T. Treu , M. Stiavelli , S. Casertano , P. Møller , G. Bertin

Velocity dispersion $\sigma$, radius $R$ and luminosity $L$ of elliptical galaxies are known to be related, leaving only two degrees of freedom and defining the so-called ``fundamental plane". In this {\em Letter} we present observational…

天体物理学 · 物理学 2016-06-08 R. Schaeffer , S. Maurogordato , A. Cappi , F. Bernardeau

Star-forming dwarfs are studied to elucidate the physical underpinnings of their fundamental plane. It is confirmed that residuals in the Tully-Fisher relation are correlated with surface brightness, but that even after accommodating the…

宇宙学与河外天体物理 · 物理学 2012-04-06 Marshall L. McCall , O. Vaduvescu , F. Pozo Nunez , A. Barr Dominguez , R. Fingerhut , E. Unda-Sanzana , Bintao Li , M. Albrecht

We use the EAGLE cosmological simulations to perform a comprehensive and systematic analysis of the $z=0.1$ Fundamental Plane (FP), the tight relation between galaxy size, mass and velocity dispersion. We first measure the total mass and…

We show that the small scatter around the Fundamental Plane (FP) of massive elliptical galaxies can be used to derive important properties of their dark and luminous matter. The central velocity dispersion sigma_0, appearing in (e.g.) the…

天体物理学 · 物理学 2009-11-07 Annamaria Borriello , Paolo Salucci , Luigi Danese

The fundamental plane (FP) has an intrinsic scatter that can not be explained purely by observational errors. Using recently available age estimates for nearby early type galaxies, we show that a galaxy's position relative to the FP depends…

天体物理学 · 物理学 2009-10-30 Duncan Forbes , Trevor Ponman , Richard Brown
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