PROGRAMME

• 10.00--10.20. D.A. Varshalovich (Ioffe Institute, St.-Petersburg).
  Welcome. Jubilees of the Russian Academy of Sciences and Neutron Star Workshops



• 10.20--10.50. D.D. Frederiks (Ioffe Institute, St.-Petersburg).
  The activity of SGR 1900+14 and SGR 1627-41 from Konus-Wind observations



• 10.50--11.10. Yu.P. Shitov (Pushchino Radioastronomical Observatory).
  Detection of the radio pulsar PSR J1907+0919 associated with the magnetar SGR 1900+14



• 11.10--11.30. V.S. Beskin (Lebedev Physical Institute, Moscow).
  On the energy loss of radio pulsars



• 11.30--11.50. A.D. Kuzmin, B.Ya. Losovsky (Pushchino Radioastronomical Observatory).
  Difference of millisecond pulsars compared to ``normal" ones by the frequency dependence of a width of integrated profiles

• 12.20--12.40. V.M. Malofeev (Pushchino Radioastronomical Observatory).
  Unique spectrum, mean and individual pulses of Geminga radio emission



• 12.40--13.00. I.F. Malov (Pushchino Radioastronomical Observatory).
  On magnetic fields and $ dot{P-P$ diagram of radio pulsars



• 13.00--13.20. V.D. Palshin, A.I. Tsygan (Ioffe Institute, St.-Petersburg).
  The effect of magnetic anomalies at the surfaces of neutron stars on X-ray luminosity of radio pulsars



• 13.20--13.40. S.V. Zharikov (Special Astrophysical Observatory).
  The distance to the millisecond pulsar PSR J1024-0719



• 13.40--14.00. T.V. Smirnova, V.I. Shishov (Pushchino Radioastronomical Observatory).
  Pulsar distances from interstellar scintillation data

• 15.00--15.20. M.E. Prokhorov, K.A. Postnov (Sternberg Astronomical Institute, Moscow).
  Close binary black holes: kick versus common envelope



• 15.20--15.40. S.B. Popov, M. Colpi, R. Turolla, A. Treves, V.M. Lipunov, M.E. Prokhorov (Sternberg Astronomical Institute, Moscow; University of Milan; University of Padova; University of Como, Italy).
  Old neutron stars in the Galaxy



• 15.40--16.00. A.G. Kuranov (Sternberg Astronomical Institute, Moscow).
  The formation of low-mass X-ray binaries with black holes from triple stars


X-RAY PULSAR

• 16.00--16.20 N.I. Shakura, M.E. Prokhorov, K.A. Postnov, N.A. Ketsaris (Sternberg Astronomical Institute, Moscow).
  On the nature of 35-day cycle in Her X-1



• 16.20--16.40. A.A. Lutovinov, S.A. Grebenev, R.A. Sunyaev (Space Research Institute, Moscow).
  Observations of wind-fed X-ray pulsars with the telescope ART-P on board GRANAT



• 16.40--17.00. A.N. Baushev, G.S. Bisnovatyi-Kogan (Space Research Institute, Moscow).
  The cyclotron emission of anisotropic electrons in the X-ray pulsars

• 17.30--18.00. Yu.N. Gnedin, S.O. Kiikov (Central Astronomical Observatory, St.-Petersburg).
  Quasi-periodic oscillations of X-ray brightness of neutron stars: new physical mechanisms



• 18.00--18.20. S.I. Kuznetsov, E.M. Churazov, M.R. Gilfanov, R.A. Sunyaev (Space Research Institute, Moscow).
  Thermal disc instability and constraints on binary system parameters in application to GRANAT / SIGMA observations of GRS 1758-258



• 18.20--18.40. D. Litvin et al. (Space Research Institute, Moscow).
  Quasiperiodic oscillations of the source A0535+262 in different spectral channels



• 18.40--19.00. E.I. Chuikin (Ioffe Institute, St.-Petersburg).
  On separation of submillisecond pulsations in hard gamma radiation of the pulsar PSR 0833-45 from observations with the GAMMA-1 telescope in autumn of 1990

• 10.00--10.40. V.S. Imshennik (ITEP, Moscow).
  Hydrodynamic model of noncentral explosion of collapsing supernovae



• 10.40--11.00. A.F. Zakharov (ITEP, Moscow).
  Rotating neutron stars and unstable models of vibrations as possible sources of gravitational radiation magnified by gravitational lenses



• 11.00--11.20. A.G. Aksenov (ITEP, Moscow).
  Gravitational radiation from a collapse of a rotating stellar core



• 11.20--11.40. A.V. Kuznetsov, N.V. Mikheev (Yaroslavl University).
  Variation of the energy and momentum of a neutrino propagating in a strongly magnetized $e^- e^+$ plasma



• 11.40--12.00. A.A. Gvozdev, I.S. Ognev (Yaroslavl University).
  Influence of neutrino reemission processes in strong magnetic field on dynamics of collapsing star envelope

• 12.30--12.50. A.D Kaminker, D.G. Yakovlev, K.P. Levenfish (Ioffe Institute, St.-Petersburg).
  Neutrino emission due to Cooper pairing of nucleons in cooling neutron stars



• 12.50--13.10. K.P. Levenfish, Yu.A. Shibanov, D.G. Yakovlev (Ioffe Institute, St.-Petersburg).
  Cooling of neutron stars with superfluid cores: theory vs. observations



• 13.10--13.30. A.B. Koptsevich, S.V. Zharikov, Yu.A. Shibanov, V.V. Sokolov, V.G. Kurt (Ioffe Institute, St.-Petersburg; Special Astrophysical Observatory; Astro Space Center of Lebedev Physical Institute, Moscow).
  Optical photometry of PSR B0656+14 and its neighbourhood



• 13.30--13.50. G.M. Beskin, V.G. Debur, V.L. Plokhotnichenko, A. Shearer (Special Astrophysical Observatory; National University of Ireland).
  High time resolution panoramic system for variability investigation of faint astronomical objects

• 15.00--15.30. I.G. Mitrofanov et al. (Space Research Institute, Moscow).
  Cosmic gamma-ray bursts in comoving reference frames



• 15.30--15.50. D.A. Anfimov et al. (Space Research Institute, Moscow).
  Spectral properties of radiation of cosmic gamma-ray bursts



• 15.50--16.10. M.S Briggs (University of Alabama, Hunstville).
  GRB 990123



• 16.10--16.30. V.V. Sokolov, V.G. Kurt, S.V. Zharikov, J. Greiner (Special Astrophysical Observatory).
  A blue object in GRB 790613 error box



• 16.30--16.50. E.V. Derishev, V.V. Kocharovsky, Vl.V. Kocharovsky (Institute for Applied Physics, Nizhnii Novgorod).
  Decoupling of neutron component and two-flow model of relativistic winds

• 17.20--17.40. V.M. Lipunov (Sternberg Astronomical Institute, Moscow).
  Gamma-ray bursts are merging relativistic stars



• 17.40--18.00. M. Litvak et al. (Space Research Institute, Moscow).
  Emission time of cosmic gamma-ray bursts



• 18.00--18.20. E.V. Derishev, V.V. Kocharovsky, Vl.V. Kocharovsky (Institute for Applied Physics, Nizhnii Novgorod).
  Neutrino transfer in a cold neutron star



• 18.20--18.40. S.I. Blinnikov, A.V. Kozyreva, I.E. Panchenko (Sternberg Astronomical Institute, Moscow).
  GRB: when do blackbody spectra look like non-thermal ones?

• G.M. Beskin, A. Shearer, A. Golden, V.L. Plokhotnichenko, V.V. Neustroev, R.M. Redfern (Special Astrophysical Observatory; National University of Ireland).
  Detection of middle-aged optical pulsars at the 6m telescope



• G.M. Beskin, V.N. Komarova, V.L. Plokhotnichenko (Special Astrophysical Observatory).
  The results of the Crab pulsar photometrical investigations with time resolution of 3.3$ mu s$



• E.V. Derishev, V.V. Kocharovsky, Vl.V. Kocharovsky (Institute for Applied Physics, Nizhnii Novgorod).
  100 GeV and sub-GeV features in the spectra of relativistic winds from compact stellar objects



• S.O. Kiikov (Central Astronomical Observatory, St.-Petersburg). Magnetocavitation model of quasi-periodic oscillations of X-ray radiation of neutron stars



• V.N. Komarova (Special Astrophysical Observatory).
  CCD-observations of ``middle-aged'' pulsars with the 6m telescope
• D.Y. Konenkov, U. Geppert (Ioffe Institute, St.-Petersburg; Astrophysikalisches Institut Potsdam).
  The effect of the neutron star crust on the evolution of a core magnetic field



• I.E. Panchenko, D.N. Drozdova, V.M. Lipunov (Sternberg Astronomical Institute, Moscow).
  Search for a pulsar-like mechanism powered by orbital motion



• A.S. Pozanenko et al. (Space Research Institute, Moscow).
  Aperiodic properties of gamma-ray bursts



• A. Sanin et al. (Space Research Institute, Moscow).
  Cosmological invariants of gamma-ray bursts



• A.N. Timokhin, G.S. Bisnovatyi-Kogan, H.C. Spruit (Sternberg Astronomical Institute, Moscow; Space Research Institute, Moscow; Max-Planck-Institut f"ur Astrophysik, Garching, Germany).
  Magnetosphere of oscillating neutron star. Nonvacuum treatment

Created: May 12 1999
Last revised: May 15, 1999