The ultraluminous X-ray source bubble in NGC 5585

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The ultraluminous X-ray source bubble in NGC 5585

Some ultraluminous X-ray sources (ULXs) are surrounded by collisionally ionized bubbles, larger and more energetic than supernova remnants: they are evidence of the powerful outflows associated with super-Eddington X-ray sources. We illustrate the most recent addition to this class: a huge (350 pc ×...

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Bibliographic Details
Main Authors:	Soria, Roberto, Pakull, M.W., Motch, C., Miller-Jones, James, Schwope, A.D., Urquhart, R.T., Ryan, M.S.
Format:	Journal Article
Language:	English
Published:	OXFORD UNIV PRESS 2021
Subjects:	Science & Technology Physical Sciences Astronomy & Astrophysics accretion, accretion discs stars: black holes ISM: bubbles ISM: jets and outflows X-rays: binaries NEARBY SPIRAL GALAXIES BLACK-HOLE CANDIDATE SUPERNOVA-REMNANTS ACCRETION DISK SPECTRAL SIGNATURES RADIO-SOURCES FAST SHOCKS JET-POWER EMISSION STELLAR
Online Access:	http://hdl.handle.net/20.500.11937/97229

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