THE NATURE OF THE X-RAY EMISSION FROM A YOUNG ACCRETING STAR PLAYS A KEY ROLE IN ITS GROWTH. THE X-RAY EMISSION OF THESE STARS HAS BEEN POSTULATED TO COME FROM THE ACCRETION SHOCK ON THE STELLAR SURFACE IN ADDITION TO THE STELLAR CORONA.
$20,153FY2021National Aeronautics and Space AdministrationNASA
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