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A discrete chemo-dynamical model of M87's globular clusters: Kinematics extending to ~ 400 kpc | Chao Li
; Ling Zhu
; R. J. Long
; Shude Mao
; Eric W. Peng
; Marc Sarzi
; Glenn van de Ven
; Hongxin Zhang
; Rui Guo
; Xiangxiang Xue
; Alessia Longobardi
; Patrick Côté
; Laura Ferrarese
; Chengze Liu
; Stephen Gwyn
; Sungsoon Lim
; Youkyung Ko
; | Date: |
19 May 2020 | Abstract: | We study the mass distribution and kinematics of the giant elliptical galaxy
M87 (NGC 4486) using discrete chemo-dynamical, axisymmetric Jeans equation
modelling. Our catalogue comprises 894 globular clusters (GCs) extending to a
projected radius of $sim 430$ kpc with line-of-sight velocities and colours,
and Multi Unit Spectroscopic Explorer (MUSE) integral field unit data within
the central $2.4$ kpc of the main galaxy. The gravitational potential for our
models is a combination of a luminous matter potential with a varying
mass-to-light ratio for the main galaxy, a supermassive black hole and a dark
matter (DM) potential with a cusped or cored DM halo. The best-fitting models
with either a cusped or a cored DM halo show no significant differences and
both are acceptable. We obtain a total mass of $(2.16 pm 0.38) imes 10^{13}
M_{odot}$ within $sim$ 400 kpc. By including the stellar mass-to-light ratio
gradient, the DM fraction increases from $sim$ 26 percent (with no gradient)
to $sim$ 73 percent within $1,R_e^{
m maj}$ (major axis of half-light
isophote, 14.2 kpc), and from $sim$ 84 percent to $sim$ 94 percent within
$5,R_e^{
m maj}$ (71.2 kpc). Red GCs have moderate rotation with $V_{
m
max}/sigma sim$ 0.4, and blue GCs have weak rotation with $V_{
m max}/sigma
sim$ 0.1. Red GCs have tangential velocity dispersion anisotropy, while blue
GCs are consistent with being nearly isotropic. Our results suggest that red
GCs are more likely to be born in-situ, while blue GCs are more likely to be
accreted. | Source: | arXiv, 2005.9410 | Services: | Forum | Review | PDF | Favorites |
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