Bright Mini-outburst Ends the 12 yr Long Activity of the Black Hole Candidate Swift J1753.5-0127

Bright Mini-outburst Ends the 12 yr Long Activity of the Black Hole Candidate Swift J1753.5-0127

© 2019. The American Astronomical Society. All rights reserved. We present optical, UV, and X-ray monitoring of the short orbital period black hole X-ray binary candidate Swift J1753.5-0127, focusing on the final stages of its 12 yr long outburst that started in 2005. From 2016 September onward, the...

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Bibliographic Details
Main Authors: Zhang, G.B., Bernardini, F., Russell, D.M., Gelfand, J.D., Lasota, J.P., Qasim, A.A., Almannaei, A., Koljonen, K.I.I., Shaw, A.W., Lewis, F., Tomsick, J.A., Plotkin, Richard, Miller-Jones, James, Maitra, D., Homan, J., Charles, P.A., Kobel, P., Perez, D., Doran, R.
Format: Journal Article
Language:English
Published: IOP PUBLISHING LTD 2019
Subjects:
Science & Technology
Physical Sciences
Astronomy & Astrophysics
accretion, accretion disks
black hole physics
X-rays: individual (Swift J1753.5-0127)
DISC INSTABILITY MODEL
X-RAY TRANSIENTS
DWARF NOVAE
MULTIWAVELENGTH OBSERVATIONS
GRO JO422+32
LIGHT CURVES
DUTY CYCLE
STATE
ULTRAVIOLET
LUMINOSITY
Online Access:http://purl.org/au-research/grants/arc/FT140101082
http://hdl.handle.net/20.500.11937/80171

Internet

http://purl.org/au-research/grants/arc/FT140101082
http://hdl.handle.net/20.500.11937/80171

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