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NASA Technical Reports Server (NTRS) 20120013290: A Giant Radio Fla...
by NASA Technical Reports Server (NTRS)
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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 gamma-ray emission,
thanks to detections by 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 gamma-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 (approx 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
greater than or equal 100 MeV) reveal renewed gamma-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 gamma-ray emission is not
exclusively related to the rare giant radio flares. A 3-
week period of gamma-ray emission is also detected when
Cyg X-3 was weakly flaring in radio, right before
transition to the radio quenched state. No gamma rays are
observed during the one-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 gamma-ray emission, implying a
connection to the accretion process, and also that the
gamma-ray activity is related to the level of radio flux
(and possibly shock formation), strengthening the
connection to the relativistic jets.
Date Published: 2016-11-11 07:43:51
Identifier: NASA_NTRS_Archive_20120013290
Item Size: 8862285
Language: english
Media Type: texts
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