Hostname: page-component-84b7d79bbc-lrf7s Total loading time: 0 Render date: 2024-07-26T05:28:43.134Z Has data issue: false hasContentIssue false
  • English
  • Français

Studying dark matter haloes with Schwarzschild modeling

Published online by Cambridge University Press:  21 March 2017

Klaudia Kowalczyk ,
Ewa L. Łokas  and
Monica Valluri
Klaudia Kowalczyk
Affiliation:
Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Bartycka 18, 00–716 Warsaw, Poland email: klaudia.kowalczyk@gmail.com, lokas@camk.edu.pl
Ewa L. Łokas
Affiliation:
Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Bartycka 18, 00–716 Warsaw, Poland email: klaudia.kowalczyk@gmail.com, lokas@camk.edu.pl
Monica Valluri
Affiliation:
Department of Astronomy, University of Michigan, 1085 South University Ave., Ann Arbor, MI 48109, USA email: mvalluri@umich.edu
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present a study exploring the reliability of recovering the mass and velocity anisotropy profiles of dark matter haloes using the Schwarzschild method of modeling galaxies.

Keywords

galaxies: dwarfgalaxies: fundamental parametersgalaxies: kinematics and dynamicsLocal Groupdark matter
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Symposium S321: Formation and Evolution of Galaxy Outskirts , March 2016 , pp. 130
Copyright
Copyright © International Astronomical Union 2017 

References

Kowalczyk, K., Łokas, E. L., & Valluri, M. 2016, Proc. of Polish Astronomical Society, in pressGoogle Scholar
Schwarzschild, M. 1979, ApJ, 232, 236 Google Scholar