T. Kallman
- An Axisymmetric, Hydrodynamical Model for the Torus Wind in Active Galactic Nuclei. II. X‐Ray–Excited Funnel Flow
2008/10/24 by A. Dorodnitsyn, T. Kallman, D. Proga · 1 citation
Physics and Astronomy · #Astrophysical Phenomena and Observations #Galaxies: Formation, Evolution, Phenomena #Astronomy and Astrophysical Research