WE PROPOSE TO CONDUCT A SUITE OF RADIATION MAGNETOHYDRODYNAMIC SIMULATIONS OF THESE ACCRETION COLUMNS RANGING FROM THE RELATIVELY LOW LUMINOSITY REGIME OF ACCRETING X-RAY PULSARS TO THE HIGH LUMINOSITY REGIME OF ULTRA-LUMINOUS X-RAY SOURCES.
$313,807FY2020National Aeronautics and Space AdministrationNASA
University Of California, Santa Barbara