• Nova outbursts are apparently a source f

    From ScienceDaily@1:317/3 to All on Thu Apr 14 22:30:46 2022
    Nova outbursts are apparently a source for cosmic rays

    Date:
    April 14, 2022
    Source:
    Max Planck Institute for Physics
    Summary:
    The MAGIC telescopes have observed the nova RS Ophiuchi shining
    brightly in gamma rays at extremely high energy. The Gamma rays
    emanate from protons that are accelerated to very high energies
    in the shock front following the explosion. This suggests that
    novae are also a source of the ubiquitous cosmic radiation in
    the universe which consists mainly of protons rich in energy,
    which race through space at almost the speed of light.



    FULL STORY ========================================================================== Light on, light off -- this is how one could describe the behavior of
    the nova, which goes by the name RS Ophiuchi (RS Oph). Every 15 years
    or so, a dramatic explosion occurs in the constellation of the Serpent
    Bearer. Birthplaces of a nova are systems in which two very different
    stars live in a parasitic relationship: A white dwarf, a small, burned-out
    and tremendously dense star - - a teaspoon of its matter weighs about
    1 ton -- orbits a red giant, an old star that will soon burn up.


    ==========================================================================
    The dying giant star feeds the white dwarf with matter shedding its
    outer hydrogen layer as the gas flows onto the nearby white dwarf. This
    flow of matter continues, until the white dwarf over(h)eats itself. The temperature and pressure in the newly gained stellar shells become too
    large and are flung away in a gigantic thermonuclear explosion. The dwarf
    star remains intact and the cycle begins again -- until the spectacle
    repeats itself.

    Explosion in the high-energy range It had been speculated that such
    explosions involve high energies. The two MAGIC telescopes recorded
    gamma rays with the value of 250 gigaelectronvolts (GeV), among the
    highest energies ever measured in a nova. By comparison, the radiation
    is a hundred billion times more energetic than visible light.

    MAGIC was able to make its observations following initial alerts from
    other instruments measuring at different wavelengths. "The spectacular
    eruption of the RS Ophiuchi shows that the MAGIC telescopes' fast response really pays off: It takes them no more than 30 seconds to move to a new target," said David Green, a scientist at the Max Planck Institute for
    Physics and one of the authors of the paper.

    Accelerated protons as a part of cosmic rays After the explosion, several
    shock fronts propagated through the stellar wind from the Red Giant and
    the interstellar medium surrounding the binary system.

    These shock waves work like a giant power plant in which particles
    are accelerated to near the speed of light. The combined measurements
    suggest that the gamma rays emanate from energetic protons, nuclei of
    hydrogen atoms.

    "This also makes nova outbursts a source of cosmic rays," explains
    David Green.

    "However, they tend to play the role of local heroes -- meaning to only contribute to the cosmic rays in the close neighborhood. The big players
    for cosmic rays are supernova remnants. The shock fronts created from
    stellar explosions are far more violent compared to novae.

    To fully understand the complicated interplay of violent events with
    the interstellar medium in the Milky Way, more observations like those
    reported now will be necessary. The MAGIC collaboration will therefore
    continue to look for "restless" objects in our Galaxy and beyond.


    ========================================================================== Story Source: Materials provided by
    Max_Planck_Institute_for_Physics. Note: Content may be edited for style
    and length.


    ========================================================================== Related Multimedia:
    *
    The_binary_star_system_RS_Ophiuchi:_Matter_flows_from_the_red_giant_onto
    the_white_dwarf.

    ========================================================================== Journal Reference:
    1. V. A. Acciari, S. Ansoldi, L. A. Antonelli, A. Arbet Engels,
    M. Artero,
    K. Asano, D. Baack, A. Babić, A. Baquero, U. Barres de
    Almeida, J.

    A. Barrio, I. Batković, J. Becerra Gonza'lez, W. Bednarek, L.

    Bellizzi, E. Bernardini, M. Bernardos, A. Berti, J. Besenrieder, W.

    Bhattacharyya, C. Bigongiari, A. Biland, O. Blanch, H. Bo"kenkamp,
    G.

    Bonnoli, Ž. Bosnjak, G. Busetto, R. Carosi, G. Ceribella, M.

    Cerruti, Y. Chai, A. Chilingarian, S. Cikota, S. M. Colak,
    E. Colombo, J.

    L. Contreras, J. Cortina, S. Covino, G. D'Amico, V. D'Elia,
    P. Da Vela, F. Dazzi, A. De Angelis, B. De Lotto, A. Del Popolo,
    M. Delfino, J.

    Delgado, C. Delgado Mendez, D. Depaoli, F. Di Pierro, L. Di Venere,
    E. Do Souto Espin~eira, D. Dominis Prester, A. Donini, D. Dorner,
    M. Doro, D.

    Elsaesser, V. Fallah Ramazani, L. Farin~a Alonso, A. Fattorini,
    M. V.

    Fonseca, L. Font, C. Fruck, S. Fukami, Y. Fukazawa, R. J. Garci'a
    Lo'pez, M. Garczarczyk, S. Gasparyan, M. Gaug, N. Giglietto,
    F. Giordano, P.

    Gliwny, N. Godinović, J. G. Green, D. Green, D. Hadasch,
    A. Hahn, T.

    Hassan, L. Heckmann, J. Herrera, J. Hoang, D. Hrupec, M. Hu"tten, T.

    Inada, K. Ishio, Y. Iwamura, I. Jime'nez Marti'nez, J. Jormanainen,
    L.

    Jouvin, D. Kerszberg, Y. Kobayashi, H. Kubo, J. Kushida,
    A. Lamastra, D.

    Lelas, F. Leone, E. Lindfors, L. Linhoff, S. Lombardi, F. Longo, R.

    Lo'pez-Coto, M. Lo'pez-Moya, A. Lo'pez-Oramas, S. Loporchio,
    B. Machado de Oliveira Fraga, C. Maggio, P. Majumdar, M. Makariev,
    M. Mallamaci, G.

    Maneva, M. Manganaro, K. Mannheim, L. Maraschi, M. Mariotti, M.

    Marti'nez, A. Mas Aguilar, D. Mazin, S. Menchiari, S. Mender, S.

    Mićanović, D. Miceli, T. Miener, J. M. Miranda,
    R. Mirzoyan, E.

    Molina, A. Moralejo, D. Morcuende, V. Moreno, E. Moretti,
    T. Nakamori, L.

    Nava, V. Neustroev, M. Nievas Rosillo, C. Nigro, K. Nilsson, K.

    Nishijima, K. Noda, S. Nozaki, Y. Ohtani, T. Oka, J. Otero-Santos,
    S.

    Paiano, M. Palatiello, D. Paneque, R. Paoletti, J. M. Paredes, L.

    Pavletić, P. Pen~il, M. Persic, M. Pihet, P. G. Prada
    Moroni, E.

    Prandini, C. Priyadarshi, I. Puljak, W. Rhode, M. Ribo', J. Rico, C.

    Righi, A. Rugliancich, N. Sahakyan, T. Saito, S. Sakurai,
    K. Satalecka, F. G. Saturni, B. Schleicher, K. Schmidt,
    T. Schweizer, J. Sitarek, I.

    Snidarić, D. Sobczynska, A. Spolon, A. Stamerra,
    J. Strisković, D. Strom, M. Strzys, Y. Suda, T. Surić,
    M. Takahashi, R. Takeishi, F. Tavecchio, P. Temnikov,
    T. Terzić, M. Teshima, L. Tosti, S.

    Truzzi, A. Tutone, S. Ubach, J. van Scherpenberg, G. Vanzo,
    M. Vazquez Acosta, S. Ventura, V. Verguilov, C. F. Vigorito,
    V. Vitale, I. Vovk, M.

    Will, C. Wunderlich, T. Yamamoto, D. Zarić, F. Ambrosino, M.

    Cecconi, G. Catanzaro, C. Ferrara, A. Frasca, M. Munari,
    L. Giustolisi, J. Alonso-Santiago, M. Giarrusso, U. Munari,
    P. Valisa. Proton acceleration in thermonuclear nova explosions
    revealed by gamma rays.

    Nature Astronomy, 2022; DOI: 10.1038/s41550-022-01640-z ==========================================================================

    Link to news story: https://www.sciencedaily.com/releases/2022/04/220414125109.htm

    --- up 6 weeks, 3 days, 10 hours, 51 minutes
    * Origin: -=> Castle Rock BBS <=- Now Husky HPT Powered! (1:317/3)