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  • X-Rays: Stars  (1)
  • accretion, accretion disks  (1)
  • stars: individual (AE Aquarii)  (1)
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  • 1
    Electronic Resource
    Electronic Resource
    Springer
    Space science reviews 68 (1994), S. 261-274 
    ISSN: 1572-9672
    Keywords: Stars: Activity ; Stars: Flare ; Radio Continuum: Stars ; X-Rays: Stars
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract Radio and X-ray observations of stellar flares provide the most direct probes of energy relaase particle acceleration, and energy transport on stars other than the Sun. In this review, the observational basis for our understanding of the flare phenomenon on other stars is briefly described and outstanding interpretive and theoretical issues are discussed. I shall confine my attention to objects which are “solar-like”, to the extent that they possess deep convective envelopes and display activity which is presumed to be magnetic in origin. These include pre-main sequence objects, classical flare stars, and close binaries. Future directions are briefly discussed.
    Type of Medium: Electronic Resource
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  • 2
    Electronic Resource
    Electronic Resource
    Springer
    Space science reviews 68 (1994), S. 291-292 
    ISSN: 1572-9672
    Keywords: accretion, accretion disks ; binaries ; novae, cataclysmic variables ; radio continuum: stars ; stars: individual (AE Aquarii)
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract We report the first millimetric detections of the magnetic cataclysmic variable AE Aquarii, accompanied by contemporaneous microwave observations. These data show that the time-averaged spectrum is well fit by a power-law which extends to mm wavelengths. We suggest that the spectrum is consistent with that expected from a superposition of flare-like events.
    Type of Medium: Electronic Resource
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