The ultraluminous X-ray source bubble in NGC 5585

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

Internet

http://hdl.handle.net/20.500.11937/97229

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