@Article{DantasRibeCapeCarv:2000:TwViTh,
author = "Dantas, Christiane Cordula and Ribeiro, Andr{\'e} Luis Batista
and Capelato, Hugo Vicente and Carvalho, R. R. de",
affiliation = "{} and Departamento de Matem{\'a}tica Aplicada, IMECC and
Divis{\~a}o de Astrof{\'{\i}}sica, INPE/MCT and
{Observat{\'o}rio Nacional}",
title = "The two-component virial theorem and the physical properties of
stellar systems",
journal = "Astrophysical Journal",
year = "2000",
volume = "528",
number = "1 Part 2",
pages = "L5--L8",
month = "Jan.",
keywords = "ASTROF{\'{\I}}SICA, cosmologia, teorias, mat{\'e}ria escura,
gal{\'a}xias el{\'{\i}}pticas, din{\^a}micas, gal{\'a}xia,
cin{\'e}tica, cosmology, theories, dark matter, galaxies,
elliptical galaxies, dynamics, galaxy, kinematics.",
abstract = "Motivated by present indirect evidence that galaxies are
surrounded by dark matter halos, we investigate whether their
physical properties can be described by a formulation of the
virial theorem that explicitly takes into account the
gravitational potential term representing the interaction of the
dark halo with the baryonic or luminous component. Our analysis
shows that the application of such a {"}two-component virial
theorem{"} not only accounts for the scaling relations displayed
by, in particular, elliptical galaxies, but also for the observed
properties of all virialized stellar systems, ranging from
globular clusters to galaxy clusters.",
issn = "0004-637X and 1538-4357",
label = "9859",
language = "en",
targetfile = "The two-component virial theorem and the physical properties of
stellar systems.pdf",
urlaccessdate = "29 jun. 2024"
}