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Galaxy Evolution in the Virgo Cluster

Published online by Cambridge University Press:  01 August 2006

Bernd Vollmer
Bernd Vollmer*
Affiliation:
CDS, Observatoire astronomique de Strasbourg, 11, rue de l'université, 67000 Strasbourg, France
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Abstract

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In the last years we have gained new insights on how ram pressure acts in detail on Virgo spiral galaxies. This has been possible due to the combination of new deep HI observations, deep polarized radio continuum observations, and detailed dynamical modelling (sticky particles and MHD). As a major result a first complete ram pressure stripping time sequence could be established for the Virgo cluster.

Keywords

Galaxies: clusters: individual: Virgogalaxies: interactionsgalaxies: ISMgalaxies: kinematics and dynamics
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S235: Galaxy Evolution Across the Hubble Time , August 2006 , pp. 155 - 159
Copyright
Copyright © International Astronomical Union 2007

References

Abadi, M.G., Moore, B., & Bower, R.G. 1999, MNRAS, 308, 947.CrossRefGoogle Scholar
Bothun, G.D., Schommer, R.A., & Sullivan, W.T. III 1982, 87, 731.CrossRefGoogle Scholar
Bravo-Alfaro, H., Cayatte, V., van Gorkom, J.H., & Balkowski, C. 2000, AJ, 119, 580.CrossRefGoogle Scholar
Cayatte, V., van Gorkom, J.H., Balkowski, C., & Kotanyi, C. 1990, AJ, 100, 604.CrossRefGoogle Scholar
Chamaraux, P., Balkowski, C., & Gérard, E. 1980, A&A, 83, 38.Google Scholar
Dressler, A., Smail, I., Poggianti, B.M. 1999, ApJS, 122, 51.CrossRefGoogle Scholar
Giovanelli, R. & Haynes, M.P. 1983, AJ, 88, 881.CrossRefGoogle Scholar
Gunn, J.E. & Gott, J.R. 1972, ApJ, 176, 1.CrossRefGoogle Scholar
Kenney, Jeffrey D.P., van Gorkom, J.H., & Vollmer, B. 2004, AJ, 127, 3361.CrossRefGoogle Scholar
Koopmann, R.A., Kenney, J.D.P., & Young, J. 2001, ApJS, 135, 125.CrossRefGoogle Scholar
Marcolini, A., Brighenti, F., & D'Ercole, A. 2003, MNRAS, 345, 1329.CrossRefGoogle Scholar
Oosterloo, T. & van Gorkom, J.H. 2005, A&A, 437, L19.Google Scholar
Otmianowska-Mazur, K. & Vollmer, B. 2003, A&A, 402, 879.Google Scholar
Poggianti, B.M., Smail, I., Dressler, A. 1999, ApJ, 518, 576.CrossRefGoogle Scholar
Rödiger, E. & Hensler, G. 2005, A&A, 433, 875.Google Scholar
Rödiger, E. & Brüggen, M. 2006, MNRAS, 369, 567.CrossRefGoogle Scholar
Rödiger, E., Brüggen, M., & Höft, M. 2006, MNRAS, 371, 609.CrossRefGoogle Scholar
Schulz, S. & Struck, C. 2001, MNRAS, 328, 185.CrossRefGoogle Scholar
Shibata, R., Matsushita, K., Yamasaki, N.Y., Ohashi, T., Ishida, M., Kikuchi, K., Böhringer, H., & Matsumoto, H. 2001, ApJ, 549, 228.CrossRefGoogle Scholar
Soida, M., Otmianowska-Mazur, K., Chyzy, K., & Vollmer, B. 2006, A&A, in press; astro-ph/0608292.Google Scholar
Vollmer, B., Cayatte, V., Balkowski, C., & Duschl, W.J. 2001, ApJ, 561, 708.CrossRefGoogle Scholar
Vollmer, B. & Huchtmeier, W. 2003, A&A, 406, 427.Google Scholar
Vollmer, B., Balkowski, C., Cayatte, V., van Driel, W., & Huchtmeier, W. 2004, A&A, 419, 35.Google Scholar
Vollmer, B., Beck, R., Kenney, J.D.P., & van Gorkom, J.H. 2004, AJ, 127, 3375.CrossRefGoogle Scholar
Vollmer, B., Braine, J., Combes, F., & Sofue, Y. 2005, A&A, 441, 473.Google Scholar
Vollmer, B., Soida, M., Otmianowska-Mazur, K., Kenney, J.D.P., van Gorkom, J.H., & Beck, R. 2006, A&A, 453, 883.Google Scholar