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Globular Cluster Systems in Massive Low Surface Brightness Galaxies

Published online by Cambridge University Press:  01 December 2006

Daniela Villegas
Affiliation:
ESO-Garching, Karl-Schwarzschild-Str. 2, 85748 Garching b. München, Germany email: [email protected], [email protected], [email protected], [email protected] Department of Astronomy, PUC, Vicuña Mackenna 4860, Casilla 306, Santiago 22, Chile
Markus Kissler-Patig
Affiliation:
ESO-Garching, Karl-Schwarzschild-Str. 2, 85748 Garching b. München, Germany email: [email protected], [email protected], [email protected], [email protected]
Andrés Jordán
Affiliation:
ESO-Garching, Karl-Schwarzschild-Str. 2, 85748 Garching b. München, Germany email: [email protected], [email protected], [email protected], [email protected]
Paul Goudfrooij
Affiliation:
STScI, 3700 San Martin Drive, Baltimore, MD 21218, USA email: [email protected]
Martin Zwaan
Affiliation:
ESO-Garching, Karl-Schwarzschild-Str. 2, 85748 Garching b. München, Germany email: [email protected], [email protected], [email protected], [email protected]
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Do LSB galaxies have globular clusters? If they do, how do the main features of these systems compare to the ones observed in other galaxies? What are the implications of these findings on the formation of the halo and the star formation history of LSB galaxies? These are the questions we are looking to address with this study.

We present preliminary results of an ACS/HST survey for globular clusters on massive LSB galaxies.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2007

References

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