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

Dávid Cseh, Cornelia Lang, Stéphane Corbel, Philip Kaaret, Fabien Grisé

Research output: Chapter in Book/Report/Conference proceedingConference contribution

1 Scopus citations

Abstract

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.

Original languageEnglish (US)
Title of host publicationJets at all Scales
EditorsGustavo Romero, Rashid Sunyaev, Rashid Sunyaev, Tomaso Belloni
Pages325-326
Number of pages2
EditionS275
DOIs
StatePublished - Sep 1 2010

Publication series

NameProceedings of the International Astronomical Union
NumberS275
Volume6
ISSN (Print)1743-9213
ISSN (Electronic)1743-9221

All Science Journal Classification (ASJC) codes

  • Medicine (miscellaneous)
  • Astronomy and Astrophysics
  • Nutrition and Dietetics
  • Public Health, Environmental and Occupational Health
  • Space and Planetary Science

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  • Cite this

    Cseh, D., Lang, C., Corbel, S., Kaaret, P., & Grisé, F. (2010). Large-scale radio nebula around the Ultra-Luminous X-ray Source IC 342 X-1. In G. Romero, R. Sunyaev, R. Sunyaev, & T. Belloni (Eds.), Jets at all Scales (S275 ed., pp. 325-326). (Proceedings of the International Astronomical Union; Vol. 6, No. S275). https://doi.org/10.1017/S1743921310016327