The authors show that intensity gradients from thick velocity channel maps trace magnetic fields, shocks, and self-gravitating regions in diffuse interstellar gas, though with lower accuracy than velocity gradients.
De Gruyter Studies in Mathematical Physics (Book 12), April 1, 2019
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Intensity Gradients Technique: Synergy with Velocity Gradients and Polarization Studies
The authors show that intensity gradients from thick velocity channel maps trace magnetic fields, shocks, and self-gravitating regions in diffuse interstellar gas, though with lower accuracy than velocity gradients.