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Further Observations of the Intermediate Mass Black Hole Candidate ESO 243-49 HLX-1

The brightest Ultra-Luminous X-ray source HLX-1 in the galaxy ESO 243-49 currently provides strong evidence for the existence of intermediate mass black holes. Here we present the latest multi-wavelength results on this intriguing source in X-ray, UV and radio bands. We have refined the X-ray position to sub-arcsecond accuracy. We also report the detection of UV emission that could indicate ongoing star formation in the region around HLX-1. The lack of detectable radio emission at the X-ray position strengthens the argument against a background AGN.

preprint2010arXivOpen access
S. A. FarrellM. ServillatS. R. OatesI. HeywoodO. GodetN. A. WebbD. Barret
astro-ph.COastro-ph.HE
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Open access7 authors2 topics
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S. A. FarrellM. ServillatS. R. OatesI. HeywoodO. GodetN. A. WebbD. Barret

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