Optical IFU spectroscopy of a bipolar microquasar jet in NGC 300

Optical IFU spectroscopy of a bipolar microquasar jet in NGC 300

We recently reported the discovery of a candidate jet-driving microquasar (S10) in the nearby spiral galaxy NGC 300. However, in the absence of kinematic information, we could not reliably determine the jet power or the dynamical age of the jet cavity. Here, we present optical Multi Unit Spectroscop...

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Bibliographic Details
Main Authors: McLeod, A.F., Scaringi, S., Soria, Roberto, Pakull, M.W., Urquhart, R., Maccarone, T.J., Knigge, C., Miller-Jones, James, Plotkin, Richard, Motch, C., Kruijssen, J.M.D., Schruba, A.
Format: Journal Article
Language:English
Published: OXFORD UNIV PRESS 2019
Subjects:
Science & Technology
Physical Sciences
Astronomy & Astrophysics
accretion, accretion discs
black hole physics
X-rays: binaries
X-RAY SOURCES
RELATIVISTIC JETS
RADIO JET
EMISSION
NEBULA
GALAXIES
FEEDBACK
PILLARS
SHOCKS
MODEL
astro-ph.HE
astro-ph.GA
astro-ph.SR
Online Access:http://purl.org/au-research/grants/arc/FT140101082
http://hdl.handle.net/20.500.11937/91534

Internet

http://purl.org/au-research/grants/arc/FT140101082
http://hdl.handle.net/20.500.11937/91534

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