Hostname: page-component-76fb5796d-25wd4 Total loading time: 0 Render date: 2024-04-26T06:00:45.995Z Has data issue: false hasContentIssue false
  • English
  • Français

The Ghosts of Galaxies: Tidal Debris in Clusters

Published online by Cambridge University Press:  26 May 2016

Michael D. Gregg  and
Michael J. West
Michael D. Gregg
Affiliation:
University of California, Davis and Institute of Geophysics and Planetary Physics, Lawrence Livermore National Laboratory, USA
Michael J. West
Affiliation:
University of California, Davis and Institute of Geophysics and Planetary Physics, Lawrence Livermore National Laboratory, USA

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Gravitational interactions in rich clusters can strip material from the outer parts of galaxies or even completely disrupt entire systems, giving rise to large scale, low surface brightness ghostly features stretching across intergalactic space. The nearby Coma and Centaurus clusters both have striking examples of galaxy ghosts, in the form of 100 kpc-long plumes of intergalactic debris. By searching HST archival images, we have found numerous other examples of galaxy ghosts in rich clusters at low redshift, evidence that galaxy destruction and recycling are ubiquitous, important in cluster formation and evolution, and continue to mold clusters at the present epoch. Many ghosts appear in X-ray bright clusters, perhaps signaling a connection with energetic subcluster mergers.

The fate of such material has important ramifications for cluster evolution. Our new HST WFPC2 V & I images of a portion of the Centaurus plume reveal that it contains an excess of discrete objects with −12 < MV < −6, consistent with being globular clusters or smaller dwarf galaxies. This tidally liberated material is being recycled directly into the intracluster population of stars, dwarf galaxies, globular clusters, and gas, which may have been built largely from a multitude of similar events over the life of the cluster.

Type
Part 1. Census
Information
Symposium - International Astronomical Union , Volume 217: Recycling Intergalactic and Interslettar Matter , 2004 , pp. 70 - 76
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Bertin, E. & Arnouts, S. 1996, A&AS, 117, 393.Google Scholar
Calcáneo-Roldán, C., Moore, B., Bland-Hawthorn, J., Malin, D., & Sadler, E.M. 2000, MNRAS, 314, 324.Google Scholar
Charlton, J., Knierman, K., Hunsberger, S., Gallagher, S., Whitmore, B., Kundu, A., & Hibbard, J., astro-ph/0009196.Google Scholar
Churazov, E., Gilfanov, M., Forman, W., & Jones, C. 1999, ApJ, 520, 105.Google Scholar
Dubinski, J. 1998, ApJ, 502, 141.Google Scholar
Duc, P.-A., Mirabel, I.F. 1994, A&A, 289, 83.Google Scholar
Duc, P.-A., Brinks, E., Springel, V., Pichardo, B., Weilbacher, P., & Mirabel, I.F. 2000, AJ, 120, 1238.Google Scholar
Gregg, M.D. & West, M.J. 1998, Nature, 396, 549.Google Scholar
Kavelaars, J. J. 2000, ApJ, 533, 125.Google Scholar
Lopez-Cruz, O., Yee, H.K.C., Brown, J.P., Jones, C., & Forman, W. 1997 ApJL 475, L97.Google Scholar
Whitmore, B.C., Schweizer, F. 1995, AJ, 109, 960.Google Scholar