Abstract
Observations of group and cluster galaxies reveal a large variety of interactions between galaxies and with the surrounding medium. Radio polarized emission is a very sensitive tracer of such interactions. In particular, regions of strong gas compression are often seen as polarized radio ridges, which mark regions of an enhanced magnetic field. Such enhancements can be however produced either by ram pressure or tidal effects. We present X-ray observations of a perturbed Virgo Cluster galaxy NGC 4569 and show that the analysis of the hot gas distribution and its spectral analysis in the regions where polarized radio ridges are seen, can help to distinguish between the two above scenarios.
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Acknowledgements
This work is based on observations obtained with XMM-Newton, an ESA science mission with instruments and contributions directly funded by ESA Member States and NASA. This work is supported by DLR Verbundforschung “Extraterrestrische Physik” at Ruhr-University Bochum through grant 50 OR 0801 and by the Polish Ministry of Science and Higher Education, grant 2693/H03/2006/31.
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Weżgowiec, M., Bomans, D.J., Ehle, M., Chyży, K.T., Urbanik, M., Soida, M. (2011). An X-Ray View of Polarized Radio Ridges. In: Ferreras, I., Pasquali, A. (eds) Environment and the Formation of Galaxies: 30 years later. Astrophysics and Space Science Proceedings. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-20285-8_49
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DOI: https://doi.org/10.1007/978-3-642-20285-8_49
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