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Journal Articles Monthly Notices of the Royal Astronomical Society Year : 2012

A giant radio flare from Cygnus X-3 with associated γ-ray emission

J. A. Tomsick
  • Function : Author
A. Szostek
  • Function : Author
R. H. D. Corbet
  • Function : Author
J. C. A. Miller-Jones
  • Function : Author
J. L. Richards
  • Function : Author
G. Pooley
  • Function : Author
S. Trushkin
  • Function : Author
R. Dubois
  • Function : Author
A. B. Hill
  • Function : Author
M. Kerr
  • Function : Author
W. Max-Moerbeck
A. C. S. Readhead
  • Function : Author
A. Bodaghee
  • Function : Author
V. Tudose
  • Function : Author
D. Parent
  • Function : Author
J. Wilms
  • Function : Author
K. Pottschmidt
  • Function : Author

Abstract

With frequent flaring activity of its relativistic jets, Cygnus X-3 (Cyg X-3) is one of the most active microquasars and is the only Galactic black hole candidate with confirmed high-energy γ-ray emission, thanks to detections by Fermi Large Area Telescope (Fermi/LAT) and AGILE. In 2011, Cyg X-3 was observed to transit to a soft X-ray state, which is known to be associated with high-energy γ-ray emission. We present the results of a multiwavelength campaign covering a quenched state, when radio emission from Cyg X-3 is at its weakest and the X-ray spectrum is very soft. A giant (∼20 Jy) optically thin radio flare marks the end of the quenched state, accompanied by rising non-thermal hard X-rays. Fermi/LAT observations (E≥ 100 MeV) reveal renewed γ-ray activity associated with this giant radio flare, suggesting a common origin for all non-thermal components. In addition, current observations unambiguously show that the γ-ray emission is not exclusively related to the rare giant radio flares. A three-week period of γ-ray emission is also detected when Cyg X-3 was weakly flaring in radio, right before transition to the radio quenched state. No γ-rays are observed during the ∼1-month long quenched state, when the radio flux is weakest. Our results suggest transitions into and out of the ultrasoft X-ray (radio-quenched) state trigger γ-ray emission, implying a connection to the accretion process, and also that the γ-ray activity is related to the level of radio flux (and possibly shock formation), strengthening the connection to the relativistic jets.
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insu-03612441 , version 1 (18-03-2022)

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S. Corbel, G. Dubus, J. A. Tomsick, A. Szostek, R. H. D. Corbet, et al.. A giant radio flare from Cygnus X-3 with associated γ-ray emission. Monthly Notices of the Royal Astronomical Society, 2012, 421, pp.2947-2955. ⟨10.1111/j.1365-2966.2012.20517.x⟩. ⟨insu-03612441⟩
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