In idealized MHD simulations, a transverse magnetic field broadens N V absorption lines from wind-cloud systems, while nearby strong UV backgrounds produce narrow lines from the cloud core and distant weak backgrounds leave no detectable N V line.
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Starburst heating and synthetic ion column densities in multiphase galactic outflows
In idealized MHD simulations, a transverse magnetic field broadens N V absorption lines from wind-cloud systems, while nearby strong UV backgrounds produce narrow lines from the cloud core and distant weak backgrounds leave no detectable N V line.