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

doi:10.1017/S1743921310016327

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

Astronomy & Astrophysics

Research output: Chapter in Book/Report/Conference proceeding › Conference 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 language	English (US)
Title of host publication	Jets at all Scales
Publisher	Cambridge University Press
Pages	325-326
Number of pages	2
Edition	S275
ISBN (Print)	9780521766074
DOIs	https://doi.org/10.1017/S1743921310016327
State	Published - Sep 2010

Publication series

Name	Proceedings of the International Astronomical Union
Number	S275
Volume	6
ISSN (Print)	1743-9213
ISSN (Electronic)	1743-9221

UN SDGs

This output contributes to the following UN Sustainable Development Goals (SDGs)

SDG 3 Good Health and Well-being

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

Access to Document

10.1017/S1743921310016327

Cite this

@inproceedings{84f37d4276a14af7aaff56ba4573abca,

title = "Large-scale radio nebula around the Ultra-Luminous X-ray Source IC 342 X-1",

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.",

author = "D{\'a}vid Cseh and Cornelia Lang and St{\'e}phane Corbel and Philip Kaaret and Fabien Gris{\'e}",

note = "Funding Information: The research leading to these results has received funding from the European Community{\textquoteright}s Seventh Framework Programme (FP7/2007-2013) under grant agreement number ITN 215212 {\textquotedblleft}Black Hole Universe{\textquotedblright}.",

year = "2010",

month = sep,

doi = "10.1017/S1743921310016327",

language = "English (US)",

isbn = "9780521766074",

series = "Proceedings of the International Astronomical Union",

publisher = "Cambridge University Press",

number = "S275",

pages = "325--326",

booktitle = "Jets at all Scales",

address = "United Kingdom",

edition = "S275",

}

TY - GEN

T1 - Large-scale radio nebula around the Ultra-Luminous X-ray Source IC 342 X-1

AU - Cseh, Dávid

AU - Lang, Cornelia

AU - Corbel, Stéphane

AU - Kaaret, Philip

AU - Grisé, Fabien

N1 - Funding Information: The research leading to these results has received funding from the European Community’s Seventh Framework Programme (FP7/2007-2013) under grant agreement number ITN 215212 “Black Hole Universe”.

PY - 2010/9

Y1 - 2010/9

N2 - 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.

AB - 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.

UR - https://www.scopus.com/pages/publications/84882784940

UR - https://www.scopus.com/pages/publications/84882784940#tab=citedBy

U2 - 10.1017/S1743921310016327

DO - 10.1017/S1743921310016327

M3 - Conference contribution

AN - SCOPUS:84882784940

SN - 9780521766074

T3 - Proceedings of the International Astronomical Union

SP - 325

EP - 326

BT - Jets at all Scales

PB - Cambridge University Press

ER -

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

Abstract

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