PACS numbers

95.85.Sz Gravitational radiation, magnetic fields, and other observations 97.60.Bw Supernovae 97.80.−d Binary and multiple stars
  1. A.V. Tutukov, A.M. Cherepashchuk “Evolution of close binary stars: theory and observations63 209–244 (2020)
    95.85.Sz, 97.60.−s, 97.80.−d (all)
  2. R.A. Stepanov, D.D. Sokoloff “Magnetic helicity and prospects for its observation in the interstellar medium62 1208–1213 (2019)
    47.65.Md, 95.85.Sz, 98.35.Eg (all)
  3. D.V. Bisikalo, A.G. Zhilkin, E.P. Kurbatov “Possible electromagnetic manifestations of merging black holes62 1136–1152 (2019)
    04.30.Tv, 97.10.Gz, 97.80.−d (all)
  4. A.M. Bykov “Astrophysical objects with extreme energy release: observations and theory61 805–818 (2018)
    95.30.−k, 97.60.Bw, 98.70.Sa (all)
  5. G.S. Bisnovatyi-Kogan, S.G. Moiseenko “Gravitational waves and core-collapse supernovae60 843–850 (2017)
    04.80.Nn, 95.85.Sz, 97.60.Bw, 97.60.Lf (all)
  6. A.M. Cherepashchuk “Discovery of gravitational waves: a new chapter in black hole studies59 910–917 (2016)
    04.30.−w, 97.60.Lf, 97.80.−d (all)
  7. V.M. Lipunov “Astrophysical sense of the discovery of gravitational waves59 918–928 (2016)
    04.30.−w, 95.85.Sz, 97.80.−d (all)
  8. 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)
  9. M.R. Gilfanov, R.A. Sunyaev “Radiation-dominated boundary layer between an accretion disc and the surface of a neutron star: theory and observations57 377–388 (2014)
    97.10.Gz, 97.60.Jd, 97.80.−d (all)
  10. 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)
  11. A.G. Riess “My path to the accelerating Universe56 (10) (2013)
    01.10.Fv, 95.36.+x, 97.60.Bw (all)
  12. 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)
  13. A.G. Zhilkin, D.V. Bisikalo, A.A. Boyarchuk “Flow structure in magnetic close binary stars55 115–136 (2012)
    52.30.−q, 97.10.Gz, 97.80.−d (all)
  14. A.M. Cherepashchuk “Optical investigations of X-ray binary systems54 1061–1067 (2011)
    97.60.Jd, 97.60.Lf, 97.80.−d (all)
  15. Astrophysics and astronomy (Scientific session of the Physical Sciences Division of the Russian Academy of Sciences, 26 January 2011)54 1061–1084 (2011)
    01.10.Fv, 04.20.−q, 11.27.+d, 89.60.Gg, 96.30.Cw, 96.30.Ys, 97.60.Jd, 97.60.Lf, 97.80.−d, 97.82.−j, 98.62.Sb, 98.80.Es (all)
  16. 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)
  17. V.S. Ptuskin “The origin of cosmic rays53 958–961 (2010)
    96.50.S−, 97.60.Bw, 98.62.Nx (all)
  18. A.M. Fridman, D.V. Bisikalo “The nature of accretion disks of close binary stars: overreflection instability and developed turbulence51 551–576 (2008)
    47.27.−i, 97.10.Gz, 97.80.−d (all)
  19. S.B. Popov, M.E. Prokhorov “Population synthesis in astrophysics50 1123–1146 (2007)
    97.10.−q, 97.60.Jd, 97.80.−d (all)
  20. S.N. Fabrika, P.K. Abolmasov et alUltraluminous X-ray sources in galaxies — microquasars or intermediate mass black holes49 324–329 (2006)
    01.10.Fv, 97.80.−d, 98.70.−f, 98.70.Qy (all)
  21. G.S. Bisnovatyi-Kogan “Binary and recycled pulsars: 30 years after observational discovery49 53–67 (2006)
    04.30.Db, 04.80.Cc, 97.60.Gb, 97.80.−d (all)
  22. D.Yu. Tsvetkov “Type Ib/c supernovae: new observational data45 900–902 (2002)
    97.60.Bw
  23. L.P. Grishchuk, V.M. Lipunov et alGravitational wave astronomy: in anticipation of first sources to be detected44 1–51 (2001)
    04.30.−w, 04.80.Nn, 95.55.Ym, 95.85.Sz (all)
  24. A.A. Pomeranskii, R.A. Sen’kov, I.B. Khriplovich “Spinning relativistic particles in external fields43 1055–1066 (2000)
    03.65.Pm, 12.20.−m, 04.25.Nx, 97.80.−d (all)
  25. V.B. Braginskii “Gravitational-wave astronomy: new methods of measurements43 691–699 (2000)
    04.30.−w, 04.80.Nn, 95.55.Ym, 95.85.Sz (all)
  26. V.S. Imshennik “Supernova explosions and historical chronology43 509–513 (2000)
    01.75.+m, 01.90.+g, 97.60.Bw, 98.58.Mj (all)
  27. 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)
  28. A.M. Cherepashchuk “Masses of black holes in binary stellar systems39 759–780 (1996)
    97.60.Lf, 97.80.−d (all)
  29. V.I. Dokuchaev “Birth and life of massive black holes34 (6) 447–470 (1991)
    98.62.Js, 98.54.Cm, 98.54.Aj, 97.80.−d, 97.10.Bt, 97.10.Cv (all)
  30. V.V. Nesterov, A.A. Ovchinnikov et alProblems of space astrometry. Project LOMONOSOV33 (7) 580–582 (1990)
    95.85.Sz, 97.10.Ld, 97.10.Vm (all)
  31. 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)
  32. 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)
  33. 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)
  34. 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)
  35. 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)
  36. 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)
  37. 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)
  38. 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)
  39. 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)
  40. 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)
  41. 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)
  42. I.D. Novikov “Electrodynamics of black holes and its astrophysical applications27 644–645 (1984)
    97.60.Lf, 98.62.Js, 98.54.Aj, 97.10.Kc, 97.80.−d (all)
  43. V.N. Rudenko “Relativistic experiments in gravitational fields21 893–917 (1978)
    04.80.+z, 95.85.Sz
  44. 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)
  45. 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)
  46. S.I. Vainshtein, Ya.B. Zel’dovich “Origin of Magnetic Fields in Astrophysics (Turbulent ’Dynamo’ Mechanisms)15 159–172 (1972)
    95.85.Sz, 95.30.Qd, 96.60.Hv, 97.10.Ld (all)
  47. V.L. Ginzburg “Pulsars (General Review)12 800–804 (1970)
    97.60.Gb, 97.60.Bw (all)
  48. 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)
  49. V.B. Braginskii “Gravitational radiation and the prospect of its experimental discovery8 513–521 (1966)
    04.80.Nn, 95.55.Ym, 95.30.Sf, 97.80.−d (all)
  50. 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)
  51. I.S. Shklovskii “RADIO GALAXIES5 365–400 (1962)
    98.70.Dk, 95.55.Br, 98.54.Gr, 97.60.Bw (all)
  52. 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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