The Cygnus Bubble's ultra-high-energy gamma-ray emission above 400 TeV is physically more consistent with a microquasar halo around Cygnus X-3 than with the Cygnus OB2 star-forming region.
Reports on Progress in Physics , year = 2001, month = apr, volume =
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Microquasar Cygnus X-3 as the PeVatron powering the Cygnus Bubble
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Near-IR Weak-lensing (NIRWL) Measurements in the CANDELS Fields. II. Mass Mapping and Overdensity Characterization
First near-IR weak-lensing analysis of CANDELS fields detects 12 shear-selected overdensities with masses 0.2-2.2 x 10^14 solar masses at redshifts 0.22-0.9 and mean z=0.68.
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An Inverse-Compton-Boosted Cool Core Unifies Perseus's Radio and X-ray Halos
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