Outbursts of the intermediate-mass black hole HLX-1: a wind-instability scenario

We model the intermediate-mass black hole HLX-1, using the Hubble Space Telescope, XMM–Newton and Swift. We quantify the relative contributions of a bluer component, function of X-ray irradiation, and a redder component, constant and likely coming from an old stellar population. We estimate a black...

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Bibliographic Details
Main Authors: Soria, Roberto, Musaeva, A., Wu, K., Zampieri, L., Federle, S., Urquhart, Ryan, van der Helm, E., Farrell, S.
Format: Journal Article
Published: Oxford University Press 2017
Online Access:http://hdl.handle.net/20.500.11937/54899