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Ground-based proper motions of nearby local group galaxies: A progress report for Fornax

Published online by Cambridge University Press:  13 April 2010

Rene A. Méndez
Affiliation:
Astronomy Department, Universidad de Chile, Casilla 36-D, Santiago, Chile email: [email protected], [email protected]
Edgardo Costa
Affiliation:
Astronomy Department, Universidad de Chile, Casilla 36-D, Santiago, Chile email: [email protected], [email protected]
Mario H. Pedreros
Affiliation:
Physics Department, Universidad de Tarapacá, Casilla 7-D, Arica, Chile email: [email protected]
Maximiliano Moyano
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117, Heidelberg, Germany email: [email protected]
Martin Altmann
Affiliation:
Astronomisches Rechen-Institut, Mönchhofstr. 12-14, 69120 Heidelberg, Germany email: [email protected]
Carme Gallart
Affiliation:
Instituto de Astrofísica de Canarias, Tenerife 38200, Islas Canarias, España email: [email protected]
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Abstract

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Determining the kinematics of the dwarf Spheroidal galaxies (dSph) satellites of the Milky Way (MW) is crucial to estimate the mass of our galaxy, to understand its formation process and that of its satellites, to explain the origin of stellar streams in the MW's halo that seem to be related to these satellites, and to understand the role of tidal interactions in the evolution and star formation history of low mass galaxies and of the halo of our Galaxy. In what follows we briefly explain a ground-based astrometric project that will have an impact on these issues, and present some preliminary results.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2010

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