How elevated is the dynamical-to-stellar mass ratio of the ultracompact dwarf S999?

Authors

Joachim Janz, Swinburne University of Technology
Duncan Forbes, Swinburne University of Technology
Mark Norris, Max Planck Institute for Astronomy
Jay Strader, Michigan State University
Samantha Penny, Swinburne University of Technology
Martina Fagioli, Swinburne University of Technology
Aaron Romanowsky, San Jose State UniversityFollow

Document Type

Article

Publication Date

May 2015

Publication Title

Monthly Notices of the Royal Astronomical Society

Volume

449

Issue Number

2

First Page

1716

Last Page

1730

DOI

10.1093/mnras/stv389

Keywords

galaxies: clusters: individual: Virgo Cluster, galaxies: dwarf, galaxies: star clusters: general

Disciplines

Astrophysics and Astronomy | External Galaxies

Comments

This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2015 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.This article may also be found online at this link: http://dx.doi.org/10.1093/mnras/stv389

Recommended Citation

Joachim Janz, Duncan Forbes, Mark Norris, Jay Strader, Samantha Penny, Martina Fagioli, and Aaron Romanowsky. "How elevated is the dynamical-to-stellar mass ratio of the ultracompact dwarf S999?" Monthly Notices of the Royal Astronomical Society (2015): 1716-1730. https://doi.org/10.1093/mnras/stv389