THE NEXT GENERATION VIRGO CLUSTER SURVEY. V. MODELING THE DYNAMICS OF M87 WITH THE MADE-TO-MEASURE METHOD-Reference-Cited by-同舟云学术

THE NEXT GENERATION VIRGO CLUSTER SURVEY. V. MODELING THE DYNAMICS OF M87 WITH THE MADE-TO-MEASURE METHOD

Published:2014-08-14 Issue:1 Volume:792 Page:59
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Zhu Ling^ORCID,Long R. J.,Mao Shude,Peng Eric W.,Liu Chengze,Caldwell Nelson,Li Biao,Blakeslee John P.,Côté Patrick,Cuillandre Jean-Charles,Durrell Patrick,Emsellem Eric^ORCID,Ferrarese Laura,Gwyn Stephen,Jordán Andrés,Lançon Ariane,Mei Simona,Muñoz Roberto,Puzia Thomas

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/792/i=1/a=59/pdf

Reference84 articles.

1. Dynamical models of elliptical galaxies – II. M87 and its globular clusters

2. The SAURON project - I. The panoramic integral-field spectrograph

3. The Luminosities, Sizes, and Velocity Dispersions of Brightest Cluster Galaxies: Implications for Formation History

4. Galactic Dynamics

5. THE ACS FORNAX CLUSTER SURVEY. V. MEASUREMENT AND RECALIBRATION OF SURFACE BRIGHTNESS FLUCTUATIONS AND A PRECISE VALUE OF THE FORNAX-VIRGO RELATIVE DISTANCE

Cited by 62 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Galaxy archaeology for wet mergers: Globular cluster age distributions in the Milky Way and nearby galaxies;Astronomy & Astrophysics;2024-07

2. Self-consistent dynamical models with a finite extent – IV. Wendland models based on compactly supported radial basis functions;Monthly Notices of the Royal Astronomical Society;2024-06-14

3. Investigating the dark matter halo of NGC 5128 using a discrete dynamical model;Astronomy & Astrophysics;2024-05

4. The Next Generation Virgo Cluster Survey (NGVS). XXVII. The Size and Structure of Globular Cluster Systems and Their Connection to Dark Matter Halos;The Astrophysical Journal;2024-05-01

5. Dark matter measurements combining stellar and H i kinematics: 30 per cent 1σ outliers with low dark matter content at 5Re;Monthly Notices of the Royal Astronomical Society;2024-02-05