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Advanced filters: Author: S. Arjyotha Clear advanced filters

  • Observations of a white dwarf/cool star binary that emits from X-ray to radio wavelengths, AR Sco, reveal a close binary with a 3.56-h period, pulsing in brightness with a period of 1.97 min; these pulses are so intense that the optical flux of AR Sco can increase by a factor of four within 30 s, and the pulsing is detectable at radio frequencies.

    • T. R. Marsh
    • B. T. Gänsicke
    • P. J. Wheatley
    Research
    Nature
    Volume: 537, P: 374-377