EO14042 CYCLOTRON RESONANT SCATTERING FEATURES (CRSFS OR CYCLOTRON LINES) ARE THE ONLY DIRECT WAY TO MEASURE THE B-FIELD CLOSE TO THE SURFACE OF AN ACCRETING NEUTRON STAR AND PROBE THE PHYSICS IN THE ACCRETION COLUMN. HERE WE PROPOSE A 50KS TOO

University Of Maryland, College Park, College Park MD

Investigators