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- W1610106904 abstract "We analysed the long-term variability of four microquasars (GRS 1915+105, Cyg X-1, Cyg X-3, and Sco X-1) in radio and X rays. The results of our analysis indicate the existence of two distinct modes of energy output, which we refer to as the `coupled' mode and the `flaring' mode. The coupled mode is responsible for mildly fluctuating, flat-spectrum radio emission, coupled with the X-ray emission; the flaring mode produces powerful, steep-spectrum radio flares, with no significant counterpart in X rays. We find that the fraction of time spent by a typical microquasar in the flaring mode is similar to the fraction of quasars that are radio-loud. This is consistent with the hypothesis that radio-loudness of quasars is a function of the epoch at which the source is observed." @default.
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- W1610106904 date "2007-08-28" @default.
- W1610106904 modified "2023-09-27" @default.
- W1610106904 title "Clues from microquasars to the origin of radio-loudness of quasars" @default.
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- W1610106904 doi "https://doi.org/10.22323/1.033.0087" @default.
- W1610106904 hasPublicationYear "2007" @default.
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