Serbian Astronomical Journal 2014 Issue 188, Pages: 29-36
https://doi.org/10.2298/SAJ1488029S
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Low dark matter content of the nearby early-type galaxy NGC 821
Samurović S. (Astronomical observatory, Belgrade)
Vudragović A. (Astronomical observatory, Belgrade)
Jovanović M. (Astronomical observatory, Belgrade)
Ćirković M.M. (Astronomical observatory, Belgrade)
In this paper we analyze the kinematics and dynamics of the nearby early-type
galaxy NGC 821 based on its globular clusters (GCs) and planetary nebulae
(PNe). We use PNe and GCs to extract the kinematics of NGC 821 which is then
used for the dynamical modelling based on the Jeans equation. We apply the
Jeans equation using the Newtonian mass-follows-light approach assuming
constant mass-to-light ratio and find that using such an approach we can
successfully fit the kinematic data. The inferred constant mass-to-light
ratio, 4:2 < M=LB < 12:4 present throughout the whole galaxy, implies the
lack of significant amount of dark matter. We also used three different MOND
approaches and found that we can fit the kinematic data without the need for
additional, dark, component.
Keywords: dark matter, galaxies: elliptical and lenticular, galaxies: kinematics and dynamics, galaxies: structure
Projekat Ministarstva nauke Republike Srbije,
br. 176021: Visible and invisible matter in nearby galaxies: theory and
observations