Very-high-energy particle acceleration powered by the jets of the microquasar SS 433

@article{Abeysekara2018VeryhighenergyPA,
  title={Very-high-energy particle acceleration powered by the jets of the microquasar SS 433},
  author={Anushka Udara Abeysekara and A. Albert and R. Alfaro and C. {\'A}lvarez and Juan de Dios {\'A}lvarez and Roberto Arceo and Juan Carlos Arteaga-Vel{\'a}zquez and D. Avila Rojas and H. A. Ayala Solares and E. Belmont-Moreno and Segev BenZvi and C. Brisbois and Karen S. Caballero-Mora and T. Capistr{\'a}n and A. Carrami{\~n}ana and S. Casanova and M A Castillo and U. Cotti and J. Cotzomi and S. Couti{\~n}o de Le{\'o}n and C. de Le{\'o}n and E. De la Fuente and Juan Carlos D{\'i}az-V{\'e}lez and S. Dichiara and B. L. Dingus and Michael DuVernois and R. W. Ellsworth and K. Engel and C. Espinoza and Ke Fang and H. Fleischhack and N. Fraija and A. Galv{\'a}n-G{\'a}mez and J. A. Garc{\'i}a-Gonz{\'a}lez and F. Garfias and Adrian Gonz{\'a}lez-Mu{\~n}oz and M. M. Gonz{\'a}lez and Jordan A. Goodman and Zigfried Hampel-Arias and James Patrick Harding and S. Hern{\'a}ndez and J. A. Hinton and B. Hona and Filiberto Hueyotl-Zahuantitla and C. M. Hui and P. H{\"u}ntemeyer and A. Iriarte and A. Jardin-Blicq and Vikram Joshi and Sarah Kaufmann and Payel Kar and Gerd J. Kunde and Robert J. Lauer and W. Hilary Lee and H. Le{\'o}n Vargas and Hang Li and J. T. Linnemann and A. L. Longinotti and G. Luis-Raya and R. L{\'o}pez-Coto and K. Malone and Samuel Marinelli and O. Martinez and I. Martinez-Castellanos and Jes{\'u}s Alberto Mart{\'i}nez-Castro and J. A. Matthews and Pedro Miranda-Romagnoli and E. Moreno and M. Mostaf{\'a} and A. Nayerhoda and Lukas Nellen and M. Newbold and M. U. Nisa and R. Noriega-Papaqui and Jennifer L. Pretz and E. G. P{\'e}rez-P{\'e}rez and Zhixiang Ren and C. D. Rho and C. Rivi{\`e}re and Daniel Rosa-Gonz{\'a}lez and M. Rosenberg and E. Ruiz-Velasco and Francisco Salesa Greus and A. Sandoval and M. Schneider and H. Schoorlemmer and M. Seglar Arroyo and G. Sinnis and A. Smith and R. W. Springer and P. Surajbali and Ignacio Taboada and Omar Tibolla and K. Tollefson and I. Torres and G. Vianello and L. Villase{\~n}or and Thomas Weisgarber and F. Werner and Stefan Westerhoff and Jeffrey Scott Wood and T. Yapici and Gaurang B. Yodh and A. Zepeda and H. Zhang and H. Zhou},
  journal={Nature},
  year={2018},
  volume={562},
  pages={82-85}
}
SS 433 is a binary system containing a supergiant star that is overflowing its Roche lobe with matter accreting onto a compact object (either a black hole or neutron star)1–3. Two jets of ionized matter with a bulk velocity of approximately 0.26c (where c is the speed of light in vacuum) extend from the binary, perpendicular to the line of sight, and terminate inside W50, a supernova remnant that is being distorted by the jets2,4–8. SS 433 differs from other microquasars (small-scale versions… 
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Diffuse X-ray emission around an ultraluminous X-ray pulsar
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Microquasars (MQs) are binary systems composed by a star feeding mass to a compact object through an accretion disk. The compact object, usually a black hole, launches oppositely directed jets which
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We propose that the high energy Cosmic Ray particles around the spectral turn-down commonly called the knee and up to the upturn, commonly called the ankle, mostly come from Blue Super Giant star
SS433: A massive X-ray binary in an advanced evolutionary stage
Abstract INTEGRAL IBIS/ISGRI 18–60 keV observations of SS433 performed in 2003–2011 enabled for the first time the hard X-ray phase-resolved orbital and precessional light curves and spectra to be
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Tentative evidence of spatially extended GeV emission from SS433/W50
We have analyzed ten years of the Fermi Large Area Telescope data toward the SS433/W50 region. With the latest source catalog and diffuse background models, the γ-ray excess from SS433/W50 is
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▪ Abstract Black holes of stellar mass and neutron stars in binary systems are first detected as hard X-ray sources using high-energy space telescopes. Relativistic jets in some of these compact
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Collimated outflows (jets) appear to be a ubiquitous phenomenon associated with the accretion of material onto a compact object. Despite this ubiquity, many fundamental physics aspects of jets are
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The radio nebula W50 harbours the relativistic binary system SS433, which is a source of the powerful wind and jets. The origin of W50 is wrapped in the interplay of the wind, supernova remnant and
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