The first low-mass black hole x-ray binary identified in quiescence outside of a globular cluster

The first low-mass black hole x-ray binary identified in quiescence outside of a globular cluster

The observed relation between the X-ray and radio properties of low-luminosity accreting black holes (BHs) has enabled the identification of multiple candidate black hole X-ray binaries (BHXBs) in globular clusters (GCs). Here, we report an identification of the radio source VLA J213002.08+120904 (a...

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Bibliographic Details
Main Authors: Tetarenko, B., Bahramian, A., Arnason, R., Miller-Jones, James, Repetto, S., Heinke, C., MacCarone, T., Chomiuk, L., Sivakoff, G., Strader, J., Kirsten, Franz, Vlemmings, W.
Format: Journal Article
Published: Institute of Physics Publishing 2016
Online Access:http://purl.org/au-research/grants/arc/FT140101082
http://hdl.handle.net/20.500.11937/30473

Internet

http://purl.org/au-research/grants/arc/FT140101082
http://hdl.handle.net/20.500.11937/30473

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