Pith. sign in

REVIEW

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

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1010.5072 v1 pith:SRTWJUQN submitted 2010-10-25 astro-ph.CO astro-ph.HE

D. Cseh , C. Lang , S. Corbel , P. Kaaret , F. Grise This is my paper · ORCID
classification astro-ph.COastro-ph.HE
keywords nebularadiopowersourcex-rayassociatedmicroquasarneeded
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original 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.

Discussion (0). Continue with ORCID to comment.

Pith tools