A Massive Jet Ejection Event from the Microquasar SS 433 Accompanying Rapid X-Ray Variability
arXiv:astro-ph/0509411 · doi:10.1086/498387
Abstract
Microquasars occasionally exhibit massive jet ejections which are distinct from the continuous or quasi-continuous weak jet ejections. Because those massive jet ejections are rare and short events, they have hardly been observed in X-ray so far. In this paper, the first X-ray observation of a massive jet ejection from the microquasar SS 433 with the Rossi X-ray Timing Explorer (RXTE) is reported. SS 433 undergoing a massive ejection event shows a variety of new phenomena including a QPO-like feature near 0.1 Hz, rapid time variability, and shot-like activities. The shot-like activity may be caused by the formation of a small plasma bullet. A massive jet may be consist of thousands of those plasma bullets ejected from the binary system. The size, mass, internal energy, and kinetic energy of the bullets and the massive jet are estimated.
21 pages including 5 figures, submitted to ApJ
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Cited by in corpus (10)
- Clumpy Outflow from Supercritical Accretion Flows
- The Jets and Disc of SS 433 at Super-Eddington Luminosities
- Interpretation of the 115 Day Periodic Modulation in the X-ray Flux of NGC 5408 X-1
- Comparison between RHD simulation of supercritical accretion flows and steady model with outflows
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- The Spectrum of SS 433 in the H and K Bands
- Fast optical variability of SS 433
- The supercritical accretion disk in SS433 and ultraluminous X-ray sources
- Long-term multi-frequency monitoring of microquasars
- Hard X-ray emission from the eastern jet of SS 433 powering the W50 `Manatee' nebula: Evidence for particle re-acceleration