using scuba 2 to probe variability in x ray binary jets
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Using SCUBA-2 to Probe Variability in X-ray Binary Jets Dr. Alex - PowerPoint PPT Presentation

Using SCUBA-2 to Probe Variability in X-ray Binary Jets Dr. Alex Tetarenko East Asian Observatory Studying Jets in X-ray Binaries Modeling the Time Domain broad-band spectra ? 10 1 10 3 10 5 10 7 10 9 10 11 Frequency (GHz) Tetarenko et al.


  1. Using SCUBA-2 to Probe Variability in X-ray Binary Jets Dr. Alex Tetarenko East Asian Observatory

  2. Studying Jets in X-ray Binaries Modeling the Time Domain broad-band spectra ? 10 1 10 3 10 5 10 7 10 9 10 11 Frequency (GHz) Tetarenko et al. 2019 Alex Tetarenko – UH Labs

  3. What can we learn from time domain studies of jet emission? • Map out the jet size scale • Probe jet geometry, beyond what we can accomplish with high resolution imaging • Measure compact jet speed • Probe the connection between the accretion flow and the jet Alex Tetarenko – UH Labs

  4. V404 Cygni - June 2015 Outburst • On June 15, 2015 X-ray flaring activity detected by Swift BAT, MAXI and INTEGRAL • Extraordinary mutli-wavelength flaring activity followed • Brightest BHXB outburst in the past decade Rare, bright Well-known system Close Proximity accretion state parameters Alex Tetarenko – UH Labs

  5. The Golden Data Set VLA + + JCMT SMA Unprecedented multi- + = wavelength view VLBA (9 different frequencies!) Alex Tetarenko – UH Labs

  6. The Golden Data Set: PART 1 Extreme Flaring! • Flares reach extremely bright flux levels • Lower ν are delayed, smoothed version of higher ν • (Sub-)mm substructure not visible in cm emission Time on 2015/06/22 (HH:MM) Tetarenko et al., 2017 Alex Tetarenko – UH Labs

  7. The Golden Data Set: PART 2 Credit: J. Miller-Jones Miller-Jones et al. 2019, Nature in press Alex Tetarenko – UH Labs

  8. Twin Bi-polar Ejection Model Jet Not To Scale! Accretion Disk

  9. Lab Procedure • Reduce a time-resolved JCMT SCUBA-2 observation of V404 Cygni during the extreme flaring activity of its 2015 outburst. • Make a movie of the extreme flux changes in V404 Cygni. • Work to connect jet variability properties with internal jet physics; e.g., energy, power, and magnetic field strength. Alex Tetarenko – UH Labs

  10. Additional Notes • Follow the detailed procedure in the lab writeup for creating a time domain data cube. • You will NEED to FIRST download the data! • You will NEED to have the Starlink software installed on your machine. • All coding and analysis should be done in the jupyter notebook provided. Alex Tetarenko – UH Labs

  11. What do you need to hand in? • Please email me your lab writeup, gif movie, and jupyter notebook • Please use the subject line: UH Labs XRB Variability – [NAME] • My email is: a.tetarenko@eaobservatory.org • Questions? – Email me! Thanks! Alex Tetarenko – UH Labs

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