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2005MNRAS.361..633N - Mon. Not. R. Astron. Soc., 361, 633-637 (2005/August-1)
Radio-loud flares from microquasars and radio-loudness of quasars.
NIPOTI C., BLUNDELL K.M. and BINNEY J.
Abstract (from CDS):
A typical microquasar is in the flaring mode a few per cent of the time, which is similar to the fraction of quasars that are radio-loud. Thus there may be no essential difference between radio-loud and radio-quiet quasars; radio-loudness may simply be a function of the epoch at which the source is observed.
Abstract Copyright: 2005 RAS
Journal keyword(s): accretion, accretion discs - ISM: jets and outflows - quasars: general - X-rays: binaries
Simbad objects: 5
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