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Star formation in the Galactic bulge: the role of collisions

Published online by Cambridge University Press:  01 July 2007

Mark Cropper  and
Dave Vande Putte
Mark Cropper
Affiliation:
Mullard Space Science Laboratory, University College London, Holmbury St Mary, Dorking, Surrey RH5 6NT, UK email: msc@mssl.ucl.ac.uk
Dave Vande Putte
Affiliation:
Mullard Space Science Laboratory, University College London, Holmbury St Mary, Dorking, Surrey RH5 6NT, UK email: msc@mssl.ucl.ac.uk
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Abstract

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Prompted by the possibility that we have observed star formation triggered by globular cluster and dwarf spheroidal transits through galactic disks, we have examined kinematic evidence as to whether the superstar clusters in the Galactic bulge could have been formed from such transits. From their trajectores, we cannot exclude such a possibility. We note also that the high frequency of these transits may have generated rapid star formation at early times, and that remnant cluster cores may themselves nucleate further star formation.

Keywords

galaxies: evolutiongalaxies: star clustersGalaxy: bulgestars: formation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S245: Formation and Evolution of Galaxy Bulges , July 2007 , pp. 189 - 190
Copyright
Copyright © International Astronomical Union 2008

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