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Large-scale radio nebula around the Ultra-Luminous X-ray Source IC 342 X-1

Published online by Cambridge University Press:  24 February 2011

Dávid Cseh ,
Cornelia Lang ,
Stéphane Corbel ,
Philip Kaaret  and
Fabien Grisé
Dávid Cseh
Affiliation:
Laboratoire Astrophysique des Interactions Multi-echelles (UMR 7158), CEA/DSM-CNRS-Universite Paris Diderot, CEA Saclay, F-91191 Gif sur Yvette, France email: david.cseh@cea.fr
Cornelia Lang
Affiliation:
Department of Physics and Astronomy, University of Iowa, Iowa City, IA 52242, US
Stéphane Corbel
Affiliation:
Laboratoire Astrophysique des Interactions Multi-echelles (UMR 7158), CEA/DSM-CNRS-Universite Paris Diderot, CEA Saclay, F-91191 Gif sur Yvette, France email: david.cseh@cea.fr
Philip Kaaret
Affiliation:
Department of Physics and Astronomy, University of Iowa, Iowa City, IA 52242, US
Fabien Grisé
Affiliation:
Department of Physics and Astronomy, University of Iowa, Iowa City, IA 52242, US
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Abstract

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We present discovery of a radio nebula associated with the ultraluminous X-ray source (ULX) IC 342 X-1 using the Very Large Array (VLA). Taking the surrounding nebula as a calorimeter, one can constrain the intrinsic power of the ULX source. We compare the obtained power that is needed to supply the radio nebula with the W50 nebula powered by the microquasar SS433 and with other ULXs. We find that the power required is at least two orders of magnitude greater than that needed to power radio emission from the W50 nebula associated with the microquasar SS433. In addition, we report the detection of a compact radio core at the location of the X-ray source.

Keywords

accretionaccretion disksblack hole physicsradiation mechanisms: generalISM: kinematics and dynamics

Information

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S275: Jets at all Scales , September 2010 , pp. 325 - 326
Copyright
Copyright © International Astronomical Union 2011

References

Begelman, M. C. 2002, ApJ, 568, L97Google Scholar
Colbert, E. J. M. & Mushotzky, R. F. 1999, ApJ, 519, 89Google Scholar
Dubner, G. M., Holdaway, M., Goss, W. M., & Mirabel, I. F. 1998, AJ, 116, 1842CrossRefGoogle Scholar
Feng, H. & Kaaret, P. 2009, ApJ, 696, 1712Google Scholar
Kaaret, P, Corbel, S, Prestwich, A. H., & Zezas, A. 2003, Science, 299, 365CrossRefGoogle Scholar
King, A. R., Davies, M. B., Ward, M. J., Fabbiano, G., & Elvis, M. 2001, ApJ, 552, L109CrossRefGoogle Scholar
Körding, E., Falcke, H., & Markoff, S. 2002, A&A, 382, L13Google Scholar
Körding, E., Falcke, H., & Corbel, S. 2006, A&A, 456, 439Google Scholar
Lang, C. C., Kaaret, P., Corbel, S., & Mercer, A. 2007, ApJ, 666, 79CrossRefGoogle Scholar
Miller, N. A., Mushotzky, R. F., & Neff, S. G. 2005, ApJ, 623, 109Google Scholar
Soria, R., Fender, R. P., Hannikainen, D. C., Read, A. M., & Stevens, I. R. 2006, MNRAS, 368, 1527Google Scholar