The accreting Black Hole Swift J1753.5–0127 from radio to hard X-Ray

The accreting Black Hole Swift J1753.5–0127 from radio to hard X-Ray

We report on multiwavelength measurements of the accreting black hole Swift J1753.5–0127 in the hard state at low luminosity (L ~ 2.7 × 1036 erg s−1 assuming a distance of d = 3 kpc) in 2014 April. The radio emission is optically thick synchrotron, presumably from a compact jet. We take advantage of...

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Bibliographic Details
Main Authors: Tomsick, J., Rahoui, F., Kolehmainen, M., Miller-Jones, James, Fürst, F., Yamaoka, K., Akitaya, H., Corbel, S., Coriat, M., Done, C., Gandhi, P., Harrison, F., Huang, K., Kaaret, P., Kalemci, E., Kanda, Y., Migliari, S., Miller, J., Moritani, Y., Stern, D., Uemura, M., Urata, Y.
Format: Journal Article
Published: Institute of Physics Publishing 2015
Online Access:http://purl.org/au-research/grants/arc/FT140101082
http://hdl.handle.net/20.500.11937/34569

Internet

http://purl.org/au-research/grants/arc/FT140101082
http://hdl.handle.net/20.500.11937/34569

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