PACS numbers

97.60.Bw Supernovae
  1. G.S. Bisnovatyi-Kogan, S.G. Moiseenko “Gravitational waves and core-collapse supernovae60 (8) (2017)
    04.80.Nn, 95.85.Sz, 97.60.Bw, 97.60.Lf (all)
  2. P.V. Baklanov, S.I. Blinnikov et alITEP's achievements in astrophysics59 796–806 (2016)
    01.65.+g, 97.60.Bw, 97.80.−d (all)
  3. B.P. Schmidt “The path to measuring an accelerating Universe56 (10) (2013)
    01.10.Fv, 95.36.+x, 97.60.Bw, 98.80.Es (all)
  4. A.G. Riess “My path to the accelerating Universe56 (10) (2013)
    01.10.Fv, 95.36.+x, 97.60.Bw (all)
  5. S. Perlmutter “Measuring the acceleration of the cosmic expansion using supernovae56 (10) (2013)
    01.10.Fv, 95.36.+x, 97.60.Bw, 98.80.Es (all)
  6. V.S. Imshennik “Rotational explosion mechanism for collapsing supernovae and the two-stage neutrino signal from supernova 1987A in the Large Magellanic Cloud53 1081–1092 (2010)
    95.85.Sz, 97.60.Bw, 97.80.−d (all)
  7. V.S. Ptuskin “The origin of cosmic rays53 958–961 (2010)
    96.50.S−, 97.60.Bw, 98.62.Nx (all)
  8. D.Yu. Tsvetkov “Type Ib/c supernovae: new observational data45 900–902 (2002)
    97.60.Bw
  9. V.S. Imshennik “Supernova explosions and historical chronology43 509–513 (2000)
    01.75.+m, 01.90.+g, 97.60.Bw, 98.58.Mj (all)
  10. N.V. Ardelyan, G.S. Bisnovatyi-Kogan, S.G. Moiseenko “Explosion mechanisms of supernovae: the magnetorotational model40 1076–1079 (1997)
    04.40.Dg, 95.30.−k, 97.60.Bw (all)
  11. V.G. Ryasnyĭ “Supernova shells33 (5) 393–395 (1990)
    97.60.Bw, 96.10.+i, 97.60.Gb, 97.60.Jd, 96.60.qe (all)
  12. V.L. Ginzburg, V.A. Dogel’ “Erratum: Some aspects of gamma-ray astronomy [Sov. Phys. Uspekhi 32, 358 (May 1989)]32 1117–1117 (1989)
    98.70.Rz, 98.70.Sa, 98.58.Db, 97.60.Bw, 98.62.Gq (all)
  13. V.L. Ginzburg, V.A. Dogel’ “Some aspects of gamma-ray astronomy32 385–415 (1989)
    98.70.Rz, 98.70.Sa, 98.58.Db, 97.60.Bw, 98.62.Gq (all)
  14. V.L. Dadykin, G.T. Zatsepin, O.G. Ryazhskaya “Events detected by underground detectors on February 23, 198732 459–468 (1989)
    97.10.Bt, 95.30.Sf, 97.60.Bw, 14.60.Lm, 29.40.Mc (all)
  15. A.D. Erlykin, E.A. Mamidzhanyan, V.A. Tsarev “Autumn school ’Interaction of hadrons at above-accelerator energies’32 380–383 (1989)
    96.50.sb, 96.50.sd, 97.60.Bw, 98.62.Ra, 01.40.E− (all)
  16. N.N. Chugai “Supernova in the Large Magellanic Cloud: first year of observations31 775–776 (1988)
    97.60.Bw, 98.56.Si, 97.60.Jd, 97.10.Fy, 97.10.Ri (all)
  17. G.S. Bisnovatyi-Kogan “Gravitational collapse, neutrino radiation, and supernova light curves31 776–777 (1988)
    97.60.Bw, 95.30.Sf, 95.55.Qf, 95.75.De, 97.20.Rp, 97.10.Gz (all)
  18. E.G. Berezhko, G.F. Krymskii “Acceleration of cosmic rays by shock waves31 27–51 (1988)
    52.65.Kj, 95.30.Qd, 96.50.Fm, 97.60.Bw, 98.70.Sa (all)
  19. E.G. Berezhko, G.F. Krymskii “Acceleration of cosmic rays by shock waves31 27–51 (1988)
    96.50.Fm, 98.70.Sa, 97.60.Bw, 52.65.Kj, 95.30.Qd (all)
  20. V.B. Braginskii, L.P. Grishchuk “Gravitational wave astronomy30 81–82 (1987)
    04.30.−w, 97.60.Bw, 98.80.Bp, 98.80.Cq (all)
  21. V.S. Berezinskii “High energy neutrino astrophysics28 728–730 (1985)
    96.50.sb, 97.60.Gb, 13.75.Cs, 97.60.Bw, 97.10.Cv, 97.20.Li (all)
  22. V.L. Ginzburg “The origin of Cosmic Rays (Present State of the Problem)18 795–796 (1975)
    01.10.Fv, 96.50.sb, 98.70.Sa, 97.60.Bw (all)
  23. P.V. Shcheglov “Astroclimatic Conditions in Central Asia and Kazakhstan14 792–794 (1972)
    97.30.Qt, 97.60.Bw, 95.75.De, 97.10.Ri, 98.80.Es, 97.10.Cv (all)
  24. V.L. Ginzburg “Pulsars (General Review)12 800–804 (1970)
    97.60.Gb, 97.60.Bw (all)
  25. N.S. Kardashev “Possibility of Observing Extragalactic Pulsars12 808–808 (1970)
    97.60.Gb, 97.60.Bw, 98.70.Dk, 98.54.Gr, 98.54.Aj (all)
  26. V.L. Ginzburg, S.I. Syrovatskii “Origin of cosmic rays9 223–235 (1966)
    96.50.sb, 95.30.Qd, 98.54.Gr, 97.60.Bw (all)
  27. I.S. Shklovskii “RADIO GALAXIES5 365–400 (1962)
    98.70.Dk, 95.55.Br, 98.54.Gr, 97.60.Bw (all)
  28. V.L. Ginzburg, S.I. Syrovatskii “Present status of the question of the origin of cosmic rays3 504–541 (1961)
    96.50.sb, 96.50.Dj, 97.60.Bw, 96.60.Q−, 98.70.Sa (all)
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