XRISM observation decomposes the Fe Kα line in Cygnus A into broad (3400 km/s, 0.1-0.17 pc) and narrow (440 km/s, 6-10 pc) Keplerian components attributed to the broad line region and torus.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
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UNVERDICTED 2representative citing papers
Rci-Q extends GRASP2018 with new fitting prefactors for the Flambaum-Ginges radiative potential, plus finite-nucleus self-energy corrections and the Wichmann-Kroll vacuum polarization term.
citing papers explorer
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Rci-Q: an improved QED correction model for the GRASP2018 package
Rci-Q extends GRASP2018 with new fitting prefactors for the Flambaum-Ginges radiative potential, plus finite-nucleus self-energy corrections and the Wichmann-Kroll vacuum polarization term.