Radiatively efficient accreting black holes in the hard state: the case study of H1743–322

Radiatively efficient accreting black holes in the hard state: the case study of H1743–322

In recent years, much effort has been devoted to unravelling the connection between the accretion flow and the jets in accreting compact objects. In the present work, we report new constraints on these issues, through the long-term study of the radio and X-ray behaviour of the black hole candidate H...

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Bibliographic Details
Main Authors: Coriat, M., Corbel, S., Prat, L., Miller-Jones, James, Cseh, D., Tzioumis, A., Brocksopp, C., Rodriguez, J., Fender, R., Sivakoff, G.
Format: Journal Article
Published: Wiley-Blackwell Publishing Ltd. 2011
Subjects:
accretion
X-rays: individual: H1743-322
accretion discs
radio continuum: stars
X-rays: binaries
ISM: jets and outflows
Online Access:http://onlinelibrary.wiley.com/doi/10.1111/j.1365-2966.2011.18433.x/full
http://hdl.handle.net/20.500.11937/17902

Internet

http://onlinelibrary.wiley.com/doi/10.1111/j.1365-2966.2011.18433.x/full
http://hdl.handle.net/20.500.11937/17902

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