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A Tidal Dwarf Galaxy in the Hercules Cluster?

Published online by Cambridge University Press:  26 May 2016

W. van Driel
Affiliation:
Observatoire de Paris, GEPI, Meudon, France
P.-A. Duc
Affiliation:
CEA, Service d'Astrophysique, Gif-sur-Yvette, France
P. Amram
Affiliation:
Laboratoire d'Astrophysique de Marseille, Marseille, France
F. Bournaud
Affiliation:
CEA, Service d'Astrophysique, Gif-sur-Yvette, France
C. Balkowski
Affiliation:
Observatoire de Paris, GEPI, Meudon, France
V. Cayatte
Affiliation:
Observatoire de Paris, GEPI, Meudon, France
J. M. Dickey
Affiliation:
Dept. of Astronomy, Univ. of Minnesota, Minneapolis, MN, USA
H. Hernández
Affiliation:
Arecibo Observatory, Arecibo, PR, USA
J. Iglesias-Páramo
Affiliation:
NRAO, Green Bank, WV, USA
K. O'Neil
Affiliation:
NRAO, Green Bank, WV, USA
P. Papaderos
Affiliation:
Universitäts-Sternwarte, Göttingen, Germany
J.M. Vílchez
Affiliation:
Instituto de Astrofísica de Andalucía (CSIC), Granada, Spain

Abstract

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A candidate Tidal Dwarf Galaxy, ce-61, was identified in the merger system IC 1182 in the Hercules supercluster. The multi-wavelength data we obtained so far do not prove, however, that it is kinematically detached from the IC 1182 system and gravitationally bound.

Type
Part 4. Recycling
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Braine, J., et al. 2001, A&A, 378, 51.Google Scholar
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Iglesias-Pramo, J., van Driel, W., Duc, P.-A. 2003, A&A, 406, 453.Google Scholar
van Driel, W., et al. 2003, A&A, 399, 433.Google Scholar