Literature DB >> 12364800

Large-scale, decelerating, relativistic x-ray jets from the microquasar XTE J1550-564.

S Corbel1, R P Fender, A K Tzioumis, J A Tomsick, J A Orosz, J M Miller, R Wijnands, P Kaaret.   

Abstract

We have detected, at x-ray and radio wavelengths, large-scale moving jets from the microquasar XTE J1550-564. Plasma ejected from near the black hole traveled at relativistic velocities for at least 4 years. We present direct evidence for gradual deceleration in a relativistic jet. The broadband spectrum of the jets is consistent with synchrotron emission from high-energy (up to 10 tera-electron volts) particles that were accelerated in the shock waves formed within the relativistic ejecta or by the interaction of the jets with the interstellar medium. XTE J1550-564 offers a rare opportunity to study the dynamical evolution of relativistic jets on time scales inaccessible for active galactic nuclei jets, with implications for our understanding of relativistic jets from Galactic x-ray binaries and active galactic nuclei.

Year:  2002        PMID: 12364800     DOI: 10.1126/science.1075857

Source DB:  PubMed          Journal:  Science        ISSN: 0036-8075            Impact factor:   47.728


  2 in total

1.  Chandra enables study of x-ray jets.

Authors:  Daniel Schwartz
Journal:  Proc Natl Acad Sci U S A       Date:  2010-04-08       Impact factor: 11.205

2.  A galactic microquasar mimicking winged radio galaxies.

Authors:  Josep Martí; Pedro L Luque-Escamilla; Valentí Bosch-Ramon; Josep M Paredes
Journal:  Nat Commun       Date:  2017-11-24       Impact factor: 14.919

  2 in total

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