PACS numbers

97.60.Bw Supernovae
  1. A.M. Bykov “Astrophysical objects with extreme energy release: observations and theoryPhys. Usp. 61 805–818 (2018)
    95.30.−k, 97.60.Bw, 98.70.Sa (all)
  2. G.S. Bisnovatyi-Kogan, S.G. Moiseenko “Gravitational waves and core-collapse supernovaePhys. Usp. 60 843–850 (2017)
    04.80.Nn, 95.85.Sz, 97.60.Bw, 97.60.Lf (all)
  3. P.V. Baklanov, S.I. Blinnikov et alITEP's achievements in astrophysicsPhys. Usp. 59 796–806 (2016)
    01.65.+g, 97.60.Bw, 97.80.−d (all)
  4. B.P. Schmidt “The path to measuring an accelerating UniversePhys. Usp. 56 (10) (2013)
    01.10.Fv, 95.36.+x, 97.60.Bw, 98.80.Es (all)
  5. A.G. Riess “My path to the accelerating UniversePhys. Usp. 56 (10) (2013)
    01.10.Fv, 95.36.+x, 97.60.Bw (all)
  6. S. Perlmutter “Measuring the acceleration of the cosmic expansion using supernovaePhys. Usp. 56 (10) (2013)
    01.10.Fv, 95.36.+x, 97.60.Bw, 98.80.Es (all)
  7. V.S. Imshennik “Rotational explosion mechanism for collapsing supernovae and the two-stage neutrino signal from supernova 1987A in the Large Magellanic CloudPhys. Usp. 53 1081–1092 (2010)
    95.85.Sz, 97.60.Bw, 97.80.−d (all)
  8. V.S. Ptuskin “The origin of cosmic raysPhys. Usp. 53 958–961 (2010)
    96.50.S−, 97.60.Bw, 98.62.Nx (all)
  9. D.Yu. Tsvetkov “Type Ib/c supernovae: new observational dataPhys. Usp. 45 900–902 (2002)
    97.60.Bw
  10. V.S. Imshennik “Supernova explosions and historical chronologyPhys. Usp. 43 509–513 (2000)
    01.75.+m, 01.90.+g, 97.60.Bw, 98.58.Mj (all)
  11. N.V. Ardelyan, G.S. Bisnovatyi-Kogan, S.G. Moiseenko “Explosion mechanisms of supernovae: the magnetorotational modelPhys. Usp. 40 1076–1079 (1997)
    04.40.Dg, 95.30.−k, 97.60.Bw (all)
  12. V.G. Ryasnyĭ “Supernova shellsSov. Phys. Usp. 33 (5) 393–395 (1990)
    97.60.Bw, 96.10.+i, 97.60.Gb, 97.60.Jd, 96.60.qe (all)
  13. V.L. Ginzburg, V.A. Dogel’ “Erratum: Some aspects of gamma-ray astronomy [Sov. Phys. Uspekhi 32, 358 (May 1989)]Sov. Phys. Usp. 32 1117–1117 (1989)
    98.70.Rz, 98.70.Sa, 98.58.Db, 97.60.Bw, 98.62.Gq (all)
  14. V.L. Ginzburg, V.A. Dogel’ “Some aspects of gamma-ray astronomySov. Phys. Usp. 32 385–415 (1989)
    98.70.Rz, 98.70.Sa, 98.58.Db, 97.60.Bw, 98.62.Gq (all)
  15. V.L. Dadykin, G.T. Zatsepin, O.G. Ryazhskaya “Events detected by underground detectors on February 23, 1987Sov. Phys. Usp. 32 459–468 (1989)
    97.10.Bt, 95.30.Sf, 97.60.Bw, 14.60.Lm, 29.40.Mc (all)
  16. A.D. Erlykin, E.A. Mamidzhanyan, V.A. Tsarev “Autumn school ’Interaction of hadrons at above-accelerator energies’Sov. Phys. Usp. 32 380–383 (1989)
    96.50.sb, 96.50.sd, 97.60.Bw, 98.62.Ra, 01.40.E− (all)
  17. N.N. Chugai “Supernova in the Large Magellanic Cloud: first year of observationsSov. Phys. Usp. 31 775–776 (1988)
    97.60.Bw, 98.56.Si, 97.60.Jd, 97.10.Fy, 97.10.Ri (all)
  18. G.S. Bisnovatyi-Kogan “Gravitational collapse, neutrino radiation, and supernova light curvesSov. Phys. Usp. 31 776–777 (1988)
    97.60.Bw, 95.30.Sf, 95.55.Qf, 95.75.De, 97.20.Rp, 97.10.Gz (all)
  19. E.G. Berezhko, G.F. Krymskii “Acceleration of cosmic rays by shock wavesSov. Phys. Usp. 31 27–51 (1988)
    52.65.Kj, 95.30.Qd, 96.50.Fm, 97.60.Bw, 98.70.Sa (all)
  20. E.G. Berezhko, G.F. Krymskii “Acceleration of cosmic rays by shock wavesSov. Phys. Usp. 31 27–51 (1988)
    96.50.Fm, 98.70.Sa, 97.60.Bw, 52.65.Kj, 95.30.Qd (all)
  21. V.B. Braginskii, L.P. Grishchuk “Gravitational wave astronomySov. Phys. Usp. 30 81–82 (1987)
    04.30.−w, 97.60.Bw, 98.80.Bp, 98.80.Cq (all)
  22. V.S. Berezinskii “High energy neutrino astrophysicsSov. Phys. Usp. 28 728–730 (1985)
    96.50.sb, 97.60.Gb, 13.75.Cs, 97.60.Bw, 97.10.Cv, 97.20.Li (all)
  23. V.L. Ginzburg “The origin of Cosmic Rays (Present State of the Problem)Sov. Phys. Usp. 17 795–796 (1975)
    01.10.Fv, 96.50.sb, 98.70.Sa, 97.60.Bw (all)
  24. P.V. Shcheglov “Astroclimatic Conditions in Central Asia and KazakhstanSov. Phys. Usp. 14 792–794 (1972)
    97.30.Qt, 97.60.Bw, 95.75.De, 97.10.Ri, 98.80.Es, 97.10.Cv (all)
  25. V.L. Ginzburg “Pulsars (General Review)Sov. Phys. Usp. 12 800–804 (1970)
    97.60.Gb, 97.60.Bw (all)
  26. N.S. Kardashev “Possibility of Observing Extragalactic PulsarsSov. Phys. Usp. 12 808–808 (1970)
    97.60.Gb, 97.60.Bw, 98.70.Dk, 98.54.Gr, 98.54.Aj (all)
  27. V.L. Ginzburg, S.I. Syrovatskii “Origin of cosmic raysSov. Phys. Usp. 9 223–235 (1966)
    96.50.sb, 95.30.Qd, 98.54.Gr, 97.60.Bw (all)
  28. I.S. Shklovskii “RADIO GALAXIESSov. Phys. Usp. 5 365–400 (1962)
    98.70.Dk, 95.55.Br, 98.54.Gr, 97.60.Bw (all)
  29. V.L. Ginzburg, S.I. Syrovatskii “Present status of the question of the origin of cosmic raysSov. Phys. Usp. 3 504–541 (1961)
    96.50.sb, 96.50.Dj, 97.60.Bw, 96.60.Q−, 98.70.Sa (all)
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