Science-advisor
REGISTER info/FAQ
Login
username
password
     
forgot password?
register here
 
Research articles
  search articles
  reviews guidelines
  reviews
  articles index
My Pages
my alerts
  my messages
  my reviews
  my favorites
 
 
Stat
Members: 3645
Articles: 2'506'133
Articles rated: 2609

26 April 2024
 
  » arxiv » 2005.9410

 Article overview



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
AbstractWe 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   
 
Visitor rating: did you like this article? no 1   2   3   4   5   yes

No review found.
 Did you like this article?

This article or document is ...
important:
of broad interest:
readable:
new:
correct:
Global appreciation:

  Note: answers to reviews or questions about the article must be posted in the forum section.
Authors are not allowed to review their own article. They can use the forum section.

browser Mozilla/5.0 AppleWebKit/537.36 (KHTML, like Gecko; compatible; ClaudeBot/1.0; +claudebot@anthropic.com)






ScienXe.org
» my Online CV
» Free


News, job offers and information for researchers and scientists:
home  |  contact  |  terms of use  |  sitemap
Copyright © 2005-2024 - Scimetrica