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Extraplanar gas and magnetic fields in the cluster spiral galaxy NGC 4569

Published online by Cambridge University Press:  01 August 2006

S. Ryś ,
K. T. Chyży ,
M. Weżgowiec ,
M. Ehle  and
R. Beck
S. Ryś
Affiliation:
Astronomical Observatory, Jagiellonian University, Kraków, Poland
K. T. Chyży
Affiliation:
Astronomical Observatory, Jagiellonian University, Kraków, Poland
M. Weżgowiec
Affiliation:
Astronomical Observatory, Jagiellonian University, Kraków, Poland
M. Ehle
Affiliation:
ESAC, XMM-Newton Science Operations Centre, Madrid, Spain
R. Beck
Affiliation:
Max-Planck-Institut für Radioastronomie, Bonn, Germany
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Abstract

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The Virgo Cluster spiral NGC 4569 is known for its compact starburst in the core and unusual outflow of Hα emitting gas perpendicular to the galaxy disk. Recent radio polarimetric observations with the Effelsberg telescope reveal huge magnetized outflows. Preliminary results of our XMM-Newton observations uncover not only hot gas in the disk but also an extensive X-ray envelope around it. We investigate the possibility of starburst-induced galactic outflows in various gas phases and cluster influence on the galaxy evolution.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S237: Triggered Star Formation in a Turbulent ISM , August 2006 , pp. 470
Copyright
Copyright © International Astronomical Union 2007