PACS numbers

47.27.−i Turbulent flows 97.10.Gz Accretion and accretion disks 97.80.−d Binary and multiple stars
  1. 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)
  2. V.M. Lipunov “Astrophysical sense of the discovery of gravitational waves59 918–928 (2016)
    04.30.−w, 95.85.Sz, 97.80.−d (all)
  3. 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)
  4. V.I. Klyatskin “Stochastic structure formation in random media59 67–95 (2016)
    05.40.−a, 05.45.−a, 46.65.+g, 47.27.−i (all)
  5. D.N. Razdoburdin, V.V. Zhuravlev “Transient dynamics of perturbations in astrophysical disks58 1031–1058 (2015)
    02.30.−f, 02.60.Pn, 47.32.C−, 97.10.Gz, 97.82.Jw, 98.62.Mw (all)
  6. V.V. Zhuravlev “Analytical models of relativistic accretion disks58 527–555 (2015)
    04.20.Cv, 04.70.Bw, 47.10.A−, 47.10.ad, 97.10.Gz (all)
  7. O.G. Bakunin “Stochastic instability and turbulent transport. Characteristic scales, increments, diffusion coefficients58 252–285 (2015)
    05.40.−a, 47.27.−i, 47.53.+n (all)
  8. I.I. Vigdorovich “Does the power formula describe turbulent velocity profiles in tubes? (comment on "Turbulent flows at very large Reynolds numbers: new lessons learned" [Phys. Usp. 57 250 (2014); 58 196–198 (2015)
    47.10.−g, 47.27.−i, 47.27.Ak, 47.27.Gs (all)
  9. G.I. Barenblatt, A.J. Chorin, V.M. Prostokishin “On the problem of turbulent flows in pipes at very large Reynolds numbers (reply to comment by I I Vigdorovich [Phys. Usp. 58 (2015); Usp. Fiz. Nauk 185 213 (2015)] on "Turbulent flows at very large Reynolds numbers: new lessons learned" [Phys. Usp. 57 250 (2014); Usp. Fiz. Nauk184 265 (2014)])58 199–201 (2015)
    47.27.−i, 47.27.Ak, 47.27.N− (all)
  10. G.I. Barenblatt, A.J. Chorin, V.M. Prostokishin “Corrigenda to the paper by G I Barenblatt, A J Chorin, V M Prostokishin "Turbulent flows at very large Reynolds numbers: new lessons learned" (Usp. Fiz. Nauk, March 2014, Vol. 184, No. 3, pp. 265—272)57 1248–1248 (2014)
    47.10.−g, 47.27.−i, 47.27.Ak, 47.27.Gs (all)
  11. E.P. Kurbatov, D.V. Bisikalo, P.V. Kaygorodov “On the possible turbulence mechanism in accretion disks in nonmagnetic binary stars57 787–798 (2014)
    47.20.−k, 47.27.−i, 95.30.Lz (all)
  12. M.R. Gil’fanov, R.A. Syunyaev “Radiation-dominated boundary layer between accretion disc and neutron star surface: theory and observations57 377–388 (2014)
    97.10.Gz, 97.60.Jd, 97.80.−d (all)
  13. N.I. Shakura “Academician Zeldovich and the foundations of disk accretion57 407–412 (2014)
    04.25.dg, 97.10.Gz, 97.60.Jd (all)
  14. G.I. Barenblatt, A.J. Chorin, V.M. Prostokishin “Turbulent flows at very large Reynolds numbers: new lessons learned57 250–256 (2014)
    47.10.−g, 47.27.−i, 47.27.Ak, 47.27.Gs (all)
  15. O.G. Bakunin “The role of B.B. Kadomtsev’s ideas in shaping the current understanding of turbulent transport56 1132–1149 (2013)
    05.40.−a, 47.27.−i, 47.53.+n (all)
  16. N.I. Shakura, K.A. Postnov et alQuasi-spherical subsonic accretion in X-ray pulsars56 321–346 (2013)
    95.30.Lz, 97.10.Gz, 97.80.Jp, 98.70.Qy (all)
  17. V.E. Zakharov, V.I. Karas’ “Nonequilibrium Kolmogorov-type particle distributions and their applications56 49–78 (2013)
    47.11.−j, 47.27.−i, 47.27.ek, 52.25.Dg (all)
  18. 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)
  19. A.M. Cherepashchuk “Optical investigations of X-ray binary systems54 1061–1067 (2011)
    97.60.Jd, 97.60.Lf, 97.80.−d (all)
  20. 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)
  21. V.P. Budaev, S.P. Savin, L.M. Zelenyi “Investigation of intermittency and generalized self-similarity of turbulent boundary layers in laboratory and magnetospheric plasmas: towards a quantitative definition of plasma transport features54 875–918 (2011)
    05.45.−a, 47.27.−i, 52.35.Ra (all)
  22. V.I. Klyatskin “Integral characteristics: a key to understanding structure formation in stochastic dynamic systems54 441–464 (2011)
    05.40.−a, 05.45.−a, 46.65.+g, 47.27.−i (all)
  23. 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)
  24. P.S. Landa, D.I. Trubetskov, V.A. Gusev “Delusions versus reality in some physics problems: theory and experiment52 235–255 (2009)
    01.65.+g, 47.27.−i, 84.40.Fe (all)
  25. 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)
  26. O.G. Onishchenko, O.A. Pokhotelov, N.M. Astaf’eva “Generation of large-scale eddies and zonal winds in planetary atmospheres51 577–589 (2008)
    47.27.−i, 92.10.hf, 92.60.−e (all)
  27. S.B. Popov, M.E. Prokhorov “Population synthesis in astrophysics50 1123–1146 (2007)
    97.10.−q, 97.60.Jd, 97.80.−d (all)
  28. 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)
  29. 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)
  30. L.L. Kichatinov “The differential rotation of stars48 449–467 (2005)
    47.27.−i, 47.32.−y, 97.10.−q (all)
  31. V.S. Beskin “Axisymmetric steady flows in astrophysics46 1209–1214 (2003)
    04.70.−s, 95.30.Qd, 97.10.Gz (all)
  32. 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)
  33. V.F. Kop’ev, S.A. Chernyshev “Vortex ring oscillations, the development of turbulence in vortex rings and generation of sound43 663–690 (2000)
    43.30.−k, 47.27.−i, 47.27.Sd, 47.32.−y (all)
  34. P.K. Volkov “Similarity in problems related to zero-gravity hydromechanics41 1211–1217 (1998)
    03.40.Gc, 47.27.−i
  35. A.M. Cherepashchuk “Masses of black holes in binary stellar systems39 759–780 (1996)
    97.60.Lf, 97.80.−d (all)
  36. S.K. Betyaev “Hydrodynamics: problems and paradoxes38 287–316 (1995)
    42.11.+j, 47.27.−i, 47.32.−y (all)
  37. 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)
  38. A.G. Bershadskii “Large-scale fractal structure in laboratory turbulence, astrophysics, and the ocean33 (12) 1073–1075 (1990)
    47.53.+n, 92.10.Lq, 47.27.−i, 95.30.Lz, 05.45.Df (all)
  39. S.G. Chefranov “Advances in investigating turbulence33 (11) 994–995 (1990)
    47.27.−i, 01.30.Cc (all)
  40. B.S. Kerner, V.V. Osipov “Self-organization in active distributed media: scenarios for the spontaneous formation and evolution of dissipative structures33 (9) 679–719 (1990)
    47.27.−i, 72.30.+q (all)
  41. V.A. Dogel’ “Differential rotation and stellar convection33 (5) 392–392 (1990)
    96.60.Bn, 96.60.qd, 47.27.−i, 95.30.Lz (all)
  42. V.I. Tatarskii “Criteria for the degree of chaos32 450–451 (1989)
    47.52.+j, 47.15.−x, 47.27.−i (all)
  43. 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)
  44. A.V. Gaponov-Grekhov, M.I. Rabinovich “Nonlinear dynamics of nonequilibrium media: structures and turbulence30 433–434 (1987)
    01.10.Fv, 05.45.−a, 47.27.−i, 47.52.+j (all)
  45. I.M. Kopylov “Spectral observations of binary systems with relativistic companions using the six-meter telescope29 981–983 (1986)
    97.20.Pm, 97.80.Jp, 97.10.Ri, 97.10.Gz, 97.10.Ex (all)
  46. 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)
  47. B.S. Rinkevicius “The Doppler method of measuring local velocities using lasers16 712–725 (1974)
    47.80.Cb, 47.15.−x, 41.20.Jb, 47.85.Dh, 85.60.Gz, 47.27.−i (all)
  48. V.N. Tsytovich “Development of the concepts of plasma turbulence15 632–650 (1973)
    52.35.Ra, 52.25.Fi, 47.27.−i (all)
  49. D.A. Frank-Kamenetskii “Kirill Ivanovich Shchelkin (obituary)12 305–306 (1969)
    01.60.+q, 47.40.Rs, 47.27.−i (all)
  50. 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)
  51. Ya.B. Zel’dovich, I.D. Novikov “Relativistic astrophysics. II8 522–577 (1966)
    97.10.Kc, 97.10.Cv, 97.10.Gz, 97.60.Jd, 95.30.Qd, 98.54.Aj (all)
  52. D.V. Bisikalo, A.G. Zhilkin, E.P. Kurbatov “Possible electromagnetic manifestations of merging black holes”, accepted
    04.25.dg, 04.80.Nn, 97.10.Gz, 47.40.−x (all)
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