Optical Precursors to Black Hole X-ray Binary Outbursts: An evolving synchrotron jet spectrum in Swift J1357.2-0933

Abstract

We present six years of optical monitoring of the black hole candidate X-ray binary Swift J1357.2-0933, during and since its discovery outburst in 2011. On these long timescales, the quiescent light curve is dominated by high amplitude, short term (seconds-days) variability spanning ~ 2 magnitudes, with an increasing trend of the mean flux from 2012 to 2017 that is steeper than in any other X-ray binary found to date (0.17 mag/yr). We detected the initial optical rise of the 2017 outburst of Swift J1357.2-0933, and we report that the outburst began between April 1 and 6, 2017. Such a steep optical flux rise preceding an outburst is expected according to disk instability models, but the high amplitude variability in quiescence is not. Previous studies have shown that the quiescent spectral, polarimetric and rapid variability properties of Swift J1357.2-0933 are consistent with synchrotron emission from a weak compact jet. We find that a variable optical/infrared spectrum is responsible for the brightening: a steep, red spectrum before and soon after the 2011 outburst evolves to a brighter, flatter spectrum since 2013. The evolving spectrum appears to be due to the jet spectral break shifting from the infrared in 2012 to the optical in 2013, then back to the infrared by 2016-2017 while the optical remains relatively bright. Swift J1357.2-0933 is a valuable source to study black hole jet physics at very low accretion rates, and is possibly the only quiescent source in which the optical jet properties can be regularly monitored.

Accepted to ApJ. 9 pages, 4 figures

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Cited by in corpus (7)

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• Bright mini-outburst ends the 12-year long activity of the black hole candidate Swift J1753.5-0127
• The black hole X-ray transient Swift J1357.2-0933 as seen with Swift and NuSTAR during its 2017 outburst
• Puzzling Blue Dips in the Black Hole Candidate Swift J1357.2-0933, from ULTRACAM, SALT, ATCA, Swift and NuSTAR
• A misfired outburst in the neutron star X-ray binary Centaurus X-4
• ALMA observations of A0620-00: fresh clues on the nature of quiescent black hole X-ray binary jets
• Seven reflares, a mini-outburst and an outburst : High amplitude optical variations in the black hole X-ray binary Swift J1910.2-0546