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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: [email protected], [email protected]
Ewa L. Łokas
Affiliation:
Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Bartycka 18, 00–716 Warsaw, Poland email: [email protected], [email protected]
Monica Valluri
Affiliation:
Department of Astronomy, University of Michigan, 1085 South University Ave., Ann Arbor, MI 48109, USA email: [email protected]
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Abstract

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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