HUNTING FOR NON-THERMAL X-RAY EMISSION FROM A WHITE DWARF PULSAR

  • Mori, Kaya (PI)

Project: Research project

Project Details

Description

AMONG MANY MAGNETIC CATACLYSMIC VARIABLES AR SCORII STANDS OUT AS THE ONLY KNOWN WHITE DWARF PULSAR BINARY WHERE ITS PULSED EMISSION FROM THE RADIO TO UV BANDS IS POWERED BY SYNCHROTRON EMISSION FROM RELATIVISTIC ELECTRONS INSTEAD OF MASS ACCRETION
StatusFinished
Effective start/end date9/29/209/28/21

Funding

  • Goddard Space Flight Center: US$40,228.00

ASJC Scopus Subject Areas

  • Astronomy and Astrophysics
  • Radiation
  • Physics and Astronomy(all)
  • Aerospace Engineering

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