Action-space clustering on stellar stream data
Abstract
Stream stars removed by tides from their progenitor satellite galaxy or globular cluster act as a group of test particles on neighbouring orbits, probing the gravitational field of the Milky Way. While constraints from individual streams have been shown to be susceptible to biases, combining several streams from orbits with various distances reduces these biases. We fit a common gravitational potential to multiple stellar streams simultaneously by maximizing the clustering of the stream stars in action space. We apply this technique to members of the GD-1, Palomar 5 (Pal 5), Orphan, and Helmi streams, exploiting both the individual and combined data sets. We describe the Galactic potential with a Stackel model, and vary up to five parameters simultaneously. We find that we can only constrain the enclosed mass, and that the strongest constraints come from the GD-1, Pal 5, and Orphan streams whose combined data set yields M(<20kpc)=2.96^+0.25^_-0.26_x10^11^M_{sun}_. When including the Helmi stream in the data set, the mass uncertainty increases to M(<20kpc)=3.12^+3.21^_-0.46_x10^11^M_{sun}_.
Authors 7
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Leiden University · Leiden Observatory
Affiliation as printed
Leiden Observatory, Leiden University, Niels Bohrweg 2, NL-2333 CA Leiden, the Netherlands
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Leiden University · Leiden Observatory
Affiliation as printed
Leiden Observatory, Leiden University, Niels Bohrweg 2, NL-2333 CA Leiden, the Netherlands
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Flatiron Institute · University of Pennsylvania
Affiliation as printed
Department of Physics and Astronomy, University of Pennsylvania, 209 S 33rd St, Philadelphia, PA 19104, USA
Center for Computational Astrophysics, Flatiron Institute, 162 5th Ave., New York, NY 10010, USA
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Leiden University · Leiden Observatory
Affiliation as printed
Leiden Observatory, Leiden University, Niels Bohrweg 2, NL-2333 CA Leiden, the Netherlands
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Affiliation as printed
Kapteyn Astronomical Institute, University of Groningen, PO Box 800, NL-9700 AV Groningen, the Netherlands
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Affiliation as printed
Kapteyn Astronomical Institute, University of Groningen, PO Box 800, NL-9700 AV Groningen, the Netherlands
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Affiliation as printed
Sydney Institute for Astronomy, School of Physics, The University of Sydney, Sydney, NSW 2006, Australia
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