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Radio activity in major mergings

Published online by Cambridge University Press:  06 October 2004

E. Zucca ,
T. Venturi ,
S. Giacintucci ,
S. Bardelli  and
D. Dallacasa
E. Zucca
Affiliation:
INAF-Osservatorio Astronomico di Bologna, via Ranzani 1, 40127 Bologna, Italy e-mail: elena.zucca@bo.astro.it
T. Venturi
Affiliation:
INAF-Istituto di Radioastronomia, via Gobetti 101, 40129 Bologna, Italy
S. Giacintucci
Affiliation:
INAF-Osservatorio Astronomico di Bologna, via Ranzani 1, 40127 Bologna, Italy e-mail: elena.zucca@bo.astro.it Dipartimento di Astronomia, Università di Bologna, via Ranzani 1, 40127 Bologna, Italy
S. Bardelli
Affiliation:
INAF-Osservatorio Astronomico di Bologna, via Ranzani 1, 40127 Bologna, Italy e-mail: elena.zucca@bo.astro.it
D. Dallacasa
Affiliation:
Dipartimento di Astronomia, Università di Bologna, via Ranzani 1, 40127 Bologna, Italy
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Abstract

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Cluster mergings are expected to have an influence on the radio emission of the galaxy population. We present the results of a deep radio survey in the A3558 complex in the central region of the Shapley Concentration, in order to further explore our hypothesis of a dependence of the radio luminosity function on the age of the merging.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUC195 , March 2004 , pp. 83 - 85
Copyright
© 2004 International Astronomical Union