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


Por: Abeysekara A.U., Albert A., Alfaro R., Alvarez C., Álvarez J.D., Arceo R., Arteaga-Velázquez J.C., Avila Rojas D., Ayala Solares H.A., Belmont-Moreno E., BenZvi S.Y., Brisbois C., Caballero-Mora K.S., Capistrán T., Carramiñana A., Casanova S., Castillo M., Cotti U., Cotzomi J., Coutiño de León S., De León C., De la Fuente E., Díaz-Vélez J.C., Dichiara S., Dingus B.L., DuVernois M.A., Ellsworth R.W., Engel K., Espinoza C., Fang K., Fleischhack H., Fraija N., Galván-Gámez A., García-González J.A., Garfias F., González-Muñoz A., González M.M., Goodman J.A., Hampel-Arias Z., Harding J.P., Hernandez S., Hinton J., Hona B., Hueyotl-Zahuantitla F., Hui C.M., Hüntemeyer P., Iriarte A., Jardin-Blicq A., Joshi V., Kaufmann S., Kar P., Kunde G.J., Lauer R.J., Lee W.H., León Vargas H., Li H., Linnemann J.T., Longinotti A.L., Luis-Raya G., López-Coto R., Malone K., Marinelli S.S., Martinez O., Martinez-Castellanos I., Martínez-Castro J., Matthews J.A., Miranda-Romagnoli P., Moreno E., Mostafá M., Nayerhoda A., Nellen L., Newbold M., Nisa M.U., Noriega-Papaqui R., Pretz J., Pérez-Pérez E.G., Ren Z., Rho C.D., Rivière C., Rosa-González D., Rosenberg M., Ruiz-Velasco E., Salesa Greus F., Sandoval A., Schneider M., Schoorlemmer H., Seglar Arroyo M., Sinnis G., Smith A.J., Springer R.W., Surajbali P., Taboada I., Tibolla O., Tollefson K., Torres I., Vianello G., Villaseñor L., Weisgarber T., Werner F., Westerhoff S., Wood J., Yapici T., Yodh G., Zepeda A., Zhang H., Zhou H.

Publicada: 4 oct 2018
Categoría: Multidisciplinary

Resumen:
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 of quasars that are present within our own Galaxy) in that the accretion is believed to be super-Eddington9–11, and the luminosity of the system is about 1040 ergs per second2,9,12,13. The lobes of W50 in which the jets terminate, about 40 parsecs from the central source, are expected to accelerate charged particles, and indeed radio and X-ray emission consistent with electron synchrotron emission in a magnetic field have been observed14–16. At higher energies (greater than 100 gigaelectronvolts), the particle fluxes of ?-rays from X-ray hotspots around SS 433 have been reported as flux upper limits6,17–20. In this energy regime, it has been unclear whether the emission is dominated by electrons that are interacting with photons from the cosmic microwave background through inverse-Compton scattering or by protons that are interacting with the ambient gas. Here we report teraelectronvolt ?-ray observations of the SS 433/W50 system that spatially resolve the lobes. The teraelectronvolt emission is localized to structures in the lobes, far from the centre of the system where the jets are formed. We have measured photon energies of at least 25 teraelectronvolts, and these are certainly not Doppler-boosted, because of the viewing geometry. We conclude that the emission—from radio to teraelectronvolt energies—is consistent with a single population of electrons with energies extending to at least hundreds of teraelectronvolts in a magnetic field of about 16 microgauss. © 2018, Springer Nature Limited.

Filiaciones:
Abeysekara A.U.:
 Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, United States

Albert A.:
 Physics and Theoretical Divisions, Los Alamos National Laboratory, Los Alamos, NM, United States

Alfaro R.:
 Instituto de Fisica, Universidad Nacional Autonoma de Mexico, Mexico City, Mexico

Alvarez C.:
 Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Mexico

Álvarez J.D.:
 Universidad Michoacana de San Nicolás de Hidalgo, Morelia, Mexico

Arceo R.:
 Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Mexico

Arteaga-Velázquez J.C.:
 Universidad Michoacana de San Nicolás de Hidalgo, Morelia, Mexico

Avila Rojas D.:
 Instituto de Fisica, Universidad Nacional Autonoma de Mexico, Mexico City, Mexico

Ayala Solares H.A.:
 Department of Physics, Pennsylvania State University, University Park, PA, United States

Belmont-Moreno E.:
 Instituto de Fisica, Universidad Nacional Autonoma de Mexico, Mexico City, Mexico

BenZvi S.Y.:
 Department of Physics and Astronomy, University of Rochester, Rochester, NY, United States

Brisbois C.:
 Department of Physics, Michigan Technological University, Houghton, MI, United States

Caballero-Mora K.S.:
 Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Mexico

Capistrán T.:
 Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico

Carramiñana A.:
 Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico

Casanova S.:
 Institute of Nuclear Physics Polish Academy of Sciences, IFJ-PAN, Krakow, Poland

 Max-Planck Institute for Nuclear Physics, Heidelberg, Germany

Castillo M.:
 Universidad Michoacana de San Nicolás de Hidalgo, Morelia, Mexico

Cotti U.:
 Universidad Michoacana de San Nicolás de Hidalgo, Morelia, Mexico

Cotzomi J.:
 Facultad de Ciencias Fisico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico

Coutiño de León S.:
 Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico

De León C.:
 Facultad de Ciencias Fisico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico

De la Fuente E.:
 Departamento de Física, Centro Universitario de Ciencias Exactas e Ingenierías, Universidad de Guadalajara, Guadalajara, Mexico

Díaz-Vélez J.C.:
 Departamento de Física, Centro Universitario de Ciencias Exactas e Ingenierías, Universidad de Guadalajara, Guadalajara, Mexico

 Department of Physics and Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin-Madison, Madison, WI, United States

Dichiara S.:
 Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico City, Mexico

Dingus B.L.:
 Physics and Theoretical Divisions, Los Alamos National Laboratory, Los Alamos, NM, United States

DuVernois M.A.:
 Department of Physics and Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin-Madison, Madison, WI, United States

Ellsworth R.W.:
 School of Physics, Astronomy, and Computational Sciences, George Mason University, Fairfax, VA, United States

Engel K.:
 Department of Physics, University of Maryland, College Park, MD, United States

Espinoza C.:
 Instituto de Fisica, Universidad Nacional Autonoma de Mexico, Mexico City, Mexico

Fang K.:
 Department of Astronomy, University of Maryland, College Park, MD, United States

 Joint Space-Science Institute, University of Maryland, College Park, MD, United States

Fleischhack H.:
 Department of Physics, Michigan Technological University, Houghton, MI, United States

Fraija N.:
 Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico City, Mexico

Galván-Gámez A.:
 Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico City, Mexico

García-González J.A.:
 Instituto de Fisica, Universidad Nacional Autonoma de Mexico, Mexico City, Mexico

Garfias F.:
 Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico City, Mexico

González-Muñoz A.:
 Departamento de Física, Centro Universitario de Ciencias Exactas e Ingenierías, Universidad de Guadalajara, Guadalajara, Mexico

González M.M.:
 Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico City, Mexico

Goodman J.A.:
 Department of Physics, University of Maryland, College Park, MD, United States

Hampel-Arias Z.:
 Department of Physics and Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin-Madison, Madison, WI, United States

 Inter-university Institute for High Energies, Université Libre de Bruxelles, Brussels, Belgium

Harding J.P.:
 Physics and Theoretical Divisions, Los Alamos National Laboratory, Los Alamos, NM, United States

Hernandez S.:
 Instituto de Fisica, Universidad Nacional Autonoma de Mexico, Mexico City, Mexico

Hinton J.:
 Max-Planck Institute for Nuclear Physics, Heidelberg, Germany

Hona B.:
 Department of Physics, Michigan Technological University, Houghton, MI, United States

Hueyotl-Zahuantitla F.:
 Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Mexico

Hui C.M.:
 NASA Marshall Space Flight Center, Astrophysics Office, Huntsville, AL, United States

Hüntemeyer P.:
 Department of Physics, Michigan Technological University, Houghton, MI, United States

Iriarte A.:
 Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico City, Mexico

Jardin-Blicq A.:
 Max-Planck Institute for Nuclear Physics, Heidelberg, Germany

Joshi V.:
 Max-Planck Institute for Nuclear Physics, Heidelberg, Germany

Kaufmann S.:
 Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Mexico

Kar P.:
 Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, United States

Kunde G.J.:
 Physics and Theoretical Divisions, Los Alamos National Laboratory, Los Alamos, NM, United States

Lauer R.J.:
 Department of Physics and Astronomy, University of New Mexico, Albuquerque, NM, United States

Lee W.H.:
 Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico City, Mexico

León Vargas H.:
 Instituto de Fisica, Universidad Nacional Autonoma de Mexico, Mexico City, Mexico

Li H.:
 Physics and Theoretical Divisions, Los Alamos National Laboratory, Los Alamos, NM, United States

Linnemann J.T.:
 Department of Physics and Astronomy, Michigan State University, East Lansing, MI, United States

Longinotti A.L.:
 Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico

Luis-Raya G.:
 Universidad Politecnica de Pachuca, Pachuca, Mexico

López-Coto R.:
 INFN and Universita di Padova, Padova, Italy

Malone K.:
 Department of Physics, Pennsylvania State University, University Park, PA, United States

Marinelli S.S.:
 Department of Physics and Astronomy, Michigan State University, East Lansing, MI, United States

Martinez O.:
 Facultad de Ciencias Fisico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico

Martinez-Castellanos I.:
 Department of Physics, University of Maryland, College Park, MD, United States

Martínez-Castro J.:
 Centro de Investigación en Computación, Instituto Politécnico Nacional, México City, Mexico

Matthews J.A.:
 Department of Physics and Astronomy, University of New Mexico, Albuquerque, NM, United States

Miranda-Romagnoli P.:
 Universidad Autónoma Del Estado de Hidalgo, Pachuca, Mexico

Moreno E.:
 Instituto de Fisica, Universidad Nacional Autonoma de Mexico, Mexico City, Mexico

Mostafá M.:
 Department of Physics, Pennsylvania State University, University Park, PA, United States

Nayerhoda A.:
 Institute of Nuclear Physics Polish Academy of Sciences, IFJ-PAN, Krakow, Poland

Nellen L.:
 Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, Mexico City, Mexico

Newbold M.:
 Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, United States

Nisa M.U.:
 Department of Physics and Astronomy, University of Rochester, Rochester, NY, United States

Noriega-Papaqui R.:
 Universidad Autónoma Del Estado de Hidalgo, Pachuca, Mexico

Pretz J.:
 Department of Physics, Pennsylvania State University, University Park, PA, United States

Pérez-Pérez E.G.:
 Universidad Politecnica de Pachuca, Pachuca, Mexico

Ren Z.:
 Department of Physics and Astronomy, University of New Mexico, Albuquerque, NM, United States

Rho C.D.:
 Department of Physics and Astronomy, University of Rochester, Rochester, NY, United States

Rivière C.:
 Department of Physics, University of Maryland, College Park, MD, United States

Rosa-González D.:
 Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico

Rosenberg M.:
 Department of Physics, Pennsylvania State University, University Park, PA, United States

Ruiz-Velasco E.:
 Max-Planck Institute for Nuclear Physics, Heidelberg, Germany

Salesa Greus F.:
 Institute of Nuclear Physics Polish Academy of Sciences, IFJ-PAN, Krakow, Poland

Sandoval A.:
 Instituto de Fisica, Universidad Nacional Autonoma de Mexico, Mexico City, Mexico

Schneider M.:
 Santa Cruz Institute for Particle Physics, University of California, Santa Cruz, Santa Cruz, CA, United States

Schoorlemmer H.:
 Max-Planck Institute for Nuclear Physics, Heidelberg, Germany

Seglar Arroyo M.:
 Department of Physics, Pennsylvania State University, University Park, PA, United States

Sinnis G.:
 Physics and Theoretical Divisions, Los Alamos National Laboratory, Los Alamos, NM, United States

Smith A.J.:
 Department of Physics, University of Maryland, College Park, MD, United States

Springer R.W.:
 Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, United States

Surajbali P.:
 Max-Planck Institute for Nuclear Physics, Heidelberg, Germany

Taboada I.:
 School of Physics and Center for Relativistic Astrophysics, Georgia Institute of Technology, Atlanta, GA, United States

Tibolla O.:
 Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Mexico

Tollefson K.:
 Department of Physics and Astronomy, Michigan State University, East Lansing, MI, United States

Torres I.:
 Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico

Vianello G.:
 Department of Physics, Stanford University, Stanford, CA, United States

Villaseñor L.:
 Facultad de Ciencias Fisico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico

Weisgarber T.:
 Department of Physics and Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin-Madison, Madison, WI, United States

Werner F.:
 Max-Planck Institute for Nuclear Physics, Heidelberg, Germany

Westerhoff S.:
 Department of Physics and Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin-Madison, Madison, WI, United States

Wood J.:
 Department of Physics and Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin-Madison, Madison, WI, United States

Yapici T.:
 Department of Physics and Astronomy, University of Rochester, Rochester, NY, United States

Yodh G.:
 Department of Physics and Astronomy, University of California, Irvine, Irvine, CA, United States

Zepeda A.:
 Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Mexico

 Physics Department, Centro de Investigación y de Estudios Avanzados del IPN, Mexico City, Mexico

Zhang H.:
 Department of Physics and Astronomy, Purdue University, West Lafayette, IN, United States

Zhou H.:
 Physics and Theoretical Divisions, Los Alamos National Laboratory, Los Alamos, NM, United States
ISSN: 00280836
Editorial
NATURE PUBLISHING GROUP, MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND, Reino Unido
Tipo de documento: Letter
Volumen: 562 Número: 7725
Páginas: 82-85
WOS Id: 000446187900041
ID de PubMed: 30283106