منابع مشابه
XMM − Newton observations of the eastern jet of SS 433
Context. The radio supernova remnant W50 hosts at its center the peculiar galactic X-ray binary SS 433. It shows a central spherical structure with two " ears " which are supposed to be formed by the interaction of the precessing jets of SSwith the supernova shell. Aims. A study of the spectral and spatial structure of the X-ray emission can reveal the physical conditions of the interaction of ...
متن کاملA jet - disk symbiosis model for Gamma Ray Bursts : SS 433 the next ?
We consider a jet-disk symbiosis model to explain Gamma Ray Bursts and their afterglows. It is proposed that GRBs are created inside a pre-existing jet from a neutron star which collapses to a black hole due to massive accretion. In our model we assume that the initial energy due to this transition is all deposited in the jet by magnetic fields, using fully well explored concepts from jets and ...
متن کاملAstronomy and Astrophysics a Jet-disk Symbiosis Model for Gamma Ray Bursts: Ss 433 the Next?
We consider a jet-disk symbiosis model to explain Gamma Ray Bursts and their afterglows. It is proposed that GRBs are created inside a pre-existing jet from a neutron star which collapses to a black hole due to massive accretion. In our model we assume that the initial energy due to this transition is all deposited in the jet by magnetic fields, using fully well explored concepts from jets and ...
متن کاملA Massive Jet Ejection Event from the Microquasar SS 433 Accompanying Rapid X-Ray Variability
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 reporte...
متن کاملPossible Photometric Evidence of Ejection of Bullet Like Features in the Relativistic Jet source SS 433
SS433 is well-known for its precessing twin jets having optical bullets inferred through spectroscopic observation ofHα lines. Recently, Chakrabarti et al. (2002) described processes which may be operating in accretion disk of SS433 to produce these bullets. In a recent multi-wavelength campaign, we find sharp rise in intensity in time-scales of few minutes in X-rays, IR and radio waves through...
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ژورنال
عنوان ژورنال: Monthly Notices of the Royal Astronomical Society
سال: 1979
ISSN: 0035-8711,1365-2966
DOI: 10.1093/mnras/187.1.13p