Publication List

Refereed Papers

Numbers in the last parenthesis are those of citations, which are taken from the web of science, the ADS and SCI. The maximum number is used. In some journals data are not available. (10 February, 2004)

  1. Formation of H2 and Galaxies in the Hot Universe.
    H.Takeda, H.Sato and T.Matsuda,
    Prog. Theor. Phys., 41, No.3 (1969), 840-841, (24)
  2. Hydrodynamic Behaviour of Gas Spheres with Masses of 104M to 1020M.
    T.Matsuda and H.Sato,
    Prog. Theor. Phys. 41, No.4 (1969), 1021-1040, (6)
  3. Cooling of Pre-Galactic Gas Clouds by Hydrogen Molecule.
    T.Matsuda, H.Sato and H.Takeda,
    Prog. Theor. Phys., 42, No.2 (1969), 219-233, (87)
  4. Galaxy Formation and the Primordial Turbulence in the Expanding Hot Universe.
    H.Sato, T.Matsuda and H.Takeda,
    Prog. Theor. Phys., 43, No.4 (1970), 1115-1116, (35)
  5. Evolution of Galaxies and Secular Variation of Cosmic Rays, Magnetic Fields and Turbulence.
    T.Matsuda,
    Prog. Theor. Phys., 43, No.6 (1970), 1491-1510, (4)
  6. On the Dissipation of Primordial Turbulence in the Expanding Universe.
    K.Tomita, H.Nariai, H.Sato, T.Matsuda and H.Takeda,
    Prog. Theor. Phys., 43, No.6 (1970), 1511-1525., (2)
  7. Pre-Galactic Magnetic Fields and Cosmic Rays in the Expanding Universe.
    T.Matsuda, H.Sato and H.Takeda,
    Publ. Astr. Soc. Japan, 23, No.1 (1971), 1-5, (3)
  8. Dissipation of Primordial Turbulence and Thermal History of the Universe.
    T.Matsuda, H.Sato and H.Takeda,
    Prog. Theor. Phys., 46, No.2 (1971), 416-432, (26)
  9. Evolution of the Expanding Hot Universe.
    H.Sato, T.Matsuda and H.Takeda,
    Prog. Theor. Phys. Suppl., No.49 (1972), 11-82, (10)
  10. Dynamics of the Azimuthally Dependent Solar Wind.
    T.Matsuda and T.Sakurai,
    Cosmic Electrodynamics, 3254 No.1 (1972), 97-115. (51)
  11. On the Gravitational Collapse in Brans-Dicke Theory of Gravity.
    T.Matsuda,
    Prog. Theor. Phys., 47, No.2 (1972), 738-739, (13)
  12. Cold Neutron Star Model in Brans-Dicke Theory of Gravity.
    T.Matsuda,
    Prog. Theor. Phys., 48, No.1 (1972), 341-342, (3)
  13. A Temperature Adjustment Process in a Boussinesq Fluid via a Buoyancy-Induced Meridional Circulation.
    T.Sakurai and T.Matsuda,
    J. Fluid Mech., 54, Part3 (1972), 414-421, (16)
  14. Dynamical Contraction of Rotating Gaseous Spheroids.
    T.Hara, T.Matsuda and K.Nakazawa,
    Prog. Theor. Phys., 49, No.2 (1973), 460-478, (1)
  15. The Sound Generated by Cosmic Turbulence and the Origin of Galaxies.
    T.Matsuda, H.Takeda and H.Sato,
    Prog. Theor. Phys., 49, No.5 (1973), 1770-1771, (1)
  16. Hydrodynamic Calculations of Spherical Gravitational Collapse in the Scalar-Tensor Theory of Gravity.
    T.Matsuda and H.Nariai, Prog. Theor. Phys., 49, No.4 (1973), 1195-1204, (12)
  17. Heat-Up of Rotating Stratified Fluid.
    T.Matsuda and T.Sakurai,
    J. Phys. Soc. Japan, 34, No.6 (1973), 1659-1666, (11)
  18. Gasdynamics of a Centrifugal Machine.
    T.Sakurai and T.Matsuda,
    J. Fluid Mech., 62, Part4 (1974),727-736, (50)
  19. S.-A.Sorensen, T.Matsuda and T.Sakurai,
    Prog. Theor. Phys., 52 No.1 (1974), 333-334, (2)
  20. Computer Simulations of Gas Flow Around Close Binary Systems.
    S.-A.Sorensen, T.Matsuda and T.Sakurai,
    Astrophys. Space Sc., 33 No.2(1975), 465-480, (19)
  21. Source-Sink Flow in a Gas Centrifuge.
    T.Matsuda, T.Sakurai and H.Takeda,
    J. Fluid Mech., 69, Part1 (1975), 197-208, (16)
  22. Isotope Separation by Thermally Driven Countercurrent Gas Centrifuge.
    T.Matsuda,
    J. Nucl. Sc. Tech., 12, No.8 (1975), 512-518, (7)
  23. On the Acoustic Decay of Primordial Cosmic Turbulence.
    K.Tanabe, H.Nariai, T.Matsuda and H.Takeda,
    Prog. Theor. Phys., 54, No.3 (1975), 719-729, (1)
  24. Thermally Driven Flow in a Gas Centrifuge with an Insulated Side Wall.
    T.Matsuda, K.Hashimoto and H.Takeda,
    J. Fluid Mech., 73, Part2 (1976), 389-399, (20)
  25. New Proposal for a Gas Centrifuge with Desirable Counter- Current.
    T.Matsuda,
    J. Nucl. Sc. Tech., 13, No.2 (1976), 98-99, (2)
  26. On the Formation of Large-Scale Shock Waves in Barred Galaxies.
    S.-A.Sorensen, T.Matsuda and M.Fujimoto,
    Astrophys. Sp. Sc., 43 No.2 (1976), 491-503, (98)
  27. Thermally, Mechanically or Externally Driven Flows in a Gas Centrifuge with Insulated Horizontal End Plates.
    T.Matsuda and K.Hashimoto,
    J. Fluid Mech., 78, Part2 (1976), 337-354, (22)
  28. New Proposal for a Gas Centrifuge Rotating Differentially.
    T.Matsuda,
    J. Nucl. Sc. Tech., 13, No.12 (1976), 756-757, (1)
  29. On One-Dimensional Galactic Spiral Shocks.
    A.H.Nelson and T.Matsuda,
    Mon. Not. R. astr. Soc., 179No.3 (1977), 663-670, (23)
  30. A Galactic Vacuum Cleaner?
    T.Matsuda and A.H.Nelson,
    Nature, 266, No.5603 (1977), 607-608, (11)
  31. New Proposal for a Gas Centrifuge Rotating Differentially, (II) Non-Rotating Side Wall.
    T.Matsuda,
    J. Nucl. Sc. Tech., 14, No.3 (1977), 244-245, (0)
  32. The Structure of the Stewartson Layers in a Gas Centrifuge. Part 1. Insulated End Plates.
    T.Matsuda and K.Hashimoto,
    J. Fluid Mech., 85, Part3 (1978), 433-442, (9)
  33. The Structure of the Stewartson Layers in a Gas Centrifuge.
    Part 2. Insulated Side Wall.
    T.Matsuda and H.Takeda,
    J. Fluid Mech., 85, Part3 (1978), 443-457, (10)
  34. Resonance between Primordial Gravitational Waves and Gravitationally Bound Systems.
    T.Futamase and T.Matsuda,
    Prog. Theor. Phys., 61, No.1 (1979), 86-93, (3)
  35. Resonance between Primordial Gravitational Waves and a Galaxy.
    T.Futamase and T.Matsuda,
    Prog. Theor. Phys., 61, No.5 (1979), 1320-1326, (1)
  36. Non-Linear Corrugation Waves in Spiral Galaxies.
    A.H.Nelson and T.Matsuda,
    Mon. Not. R. astr. Soc., 191No.1 (1980), 221-235, (16)
  37. Spectrum Evolution of Primordial Cosmic Turbulence.
    T.Futamase and T.Matsuda,
    Mon. Not. R. astr. Soc., 192 No.1 (1980), 113-126, (1)
  38. Meridional Flow of Compressible Fluid in a Rapidly Rotating Short Cylinder.
    K.Hashimoto and T.Matsuda,
    J. Phys. Soc. Japan, 49, No.2 (1980), 779-786.
  39. Response of Gas to an Ovally Deformed Gravitational Potential of a Disk Galaxy.
    T.Matsuda and H.Isaka,
    Prog. Theor. Phys., 64, No.4 (1980), 1265-1279, (21)
  40. Galactic Shock Waves and Corrugation Waves.
    T.Matsuda,
    Prog. Theor. Phys. Suppl. No.70 (1982)254 249-260, (2)
  41. Gaseous Spiral Arms Produced by Oval Distortions in Disk Galaxies.
    S.-A.Sorensen and T.Matsuda,
    Mon. Not. R. astr. Soc., 198 No.3 (1982), 865-872, (12)
  42. T.Matsuda and K.Nakagawa,
    A new type of boundary layer in a rapidly rotating gas
    J. Fluid Mech., 126 (1983), 431-442, (4)
  43. Meteorology in a Space Colony.
    T.Matsuda,
    J. Phys. Soc. Japan, 52, No.6 (1983), 1904-1907.
  44. Flows in a Rotating Cylinder with a Sloping Bottom.
    K.Nakagawa, H.Takeda and T.Matsuda,
    J. Phys. Soc. Japan, 52, No.11 (1983), 3766-3772.
  45. Mass and Angular Momentum Loss from Contact Binary Systems.
    K.Sawada, I.Hachisu and T.Matsuda,
    Mon. Not. R. astr. Soc., 206, No.3 (1984), 673-690, (26)
  46. Topology of Supercluster-Void Structure.
    T.Matsuda and E.Shima,
    Prog. Theor. Phys., 71, No.4 (1984), 855-858, (13)
  47. Statistical Formulation of Electromagnetism in the Expanding Universe and Arrow of Time.
    T.Futamase and T.Matsuda,
    Prog. Theor. Phys., 72, No.1 (1984), 38-46, (1)
  48. Galactic Spiral Shocks in a Corrugated Gas Disk.
    A.H.Nelson, T.Johns and T.Matsuda, Mon. Not. R. astr. Soc., 210, No.2 (1984), 381-392, (2)
  49. Drag on a Gravitating Sphere Moving through a Gas.
    H.Takeda, T.Matsuda, K.Sawada and C.Hayashi,
    Prog. Theor. Phys., 74, No.2 (1985), 272-287, (34)
  50. Hydrodynamic Calculations of Axisymmetric Accretion Flow.
    E.Shima, T.Matsuda, H.Takeda and K.Sawada,
    Mon. Not. R. astr. Soc., 217, No.2 (1985),367-386, (93)
  51. Spiral shocks on a Roche lobe over-flow in a semi-detached binary system.
    K.Sawada, T.Matsuda and I.Hachisu,
    Mon. Not. R. astr. Soc., 219, No.1 (1986), 75-88, (127)
  52. Accretion Shocks in a Close Binary System.
    K.Sawada, T.Matsuda and I.Hachisu,
    Mon. Not. R. astr. Soc., 221, No.3 (1986), 679-686, (46)
  53. Interaction between a Stellar Wind and an Accretion Flow.
    E.Shima, T.Matsuda and T.Inaguchi,
    Mon. Not. R. astr. Soc., 221, No.3 (1986), 687-706, (22)
  54. Rocket Effect on a Gravitating Mass-Losing Object.
    T.Inaguchi, T.Matsuda and E.Shima,
    Mon. Not. R. astr. Soc., 223, No.1 (1986), 129-138, (8)
  55. Is the Standard Accretion Disc Model Invulnerable?
    K.Sawada, T.Matsuda, M.Inoue and I.Hachisu,
    Mon. Not. R. astr. Soc., 224, No.2 (1987), 307-322., (59)
  56. Spinup and Spindown of an Accreting Compact Object.
    T.Matsuda, M.Inoue and K.Sawada,
    Mon. Not. R. astr. Soc., 226, No.4 (1987), 785-811, (65)
  57. A Reinvestigation of Gas Responce to an Ovally Deformed Gravitational Potential.
    T.Matsuda, M.Inoue, K.Sawada, E.Shima and K.Wakamatsu,
    Mon. Not. R. astr. Soc., 229, No.2 (1987), 295-314, (35)
  58. Spiral Shocks and Accretion in Disks.
    H.C.Spruit, T.Matsuda, M.Inoue and K.Sawada,
    Mon. Not. R. astr. Soc., 229, No.3 (1987), 517-527, (83)
  59. A Time-symmetric Universe Model and its Observational Implication.
    T.Futamase and T.Matsuda,
    Nuovo Cimento, 100B, No.2 (1987), 277-287, (1)
  60. A Divergence-free Approximation of the Equation of Motion for a Relativistic Classical Charged Particle
    T.Futamase and T.Matsuda,
    Nuovo Cimento, 102B, No.3 (1988), 309-314, (1)
  61. Numerical Simulation of Axisymmetric Adiabatic Flow Past a Gravitating Solid Sphere.
    T.Matsuda, N.Sekino, E.Shima and K.Sawada,
    Mon. Not. R. astr. Soc., 236, No.4 (1989), 817-828, (5)
  62. Three-dimensional Numerical Simulation of Flows past Scoops in a Gas Centrifuge.
    T.Matsuda, N.Tamura and K.Sawada,
    J. Fluid Mech., 201 (1989), 203-221, (1)
  63. Numerical Simulations of Interaction between Stellar Wind and Interstellar Medium.
    T.Matsuda, Y.Fujimoto, E.Shima, K.Sawada and T.Inaguchi,
    Prog. Theor. Phys., 81, No.4 (1989) April 25, 810-822, (37)
  64. Pressure Gradient Torque in Highly Supersonic Non- axisymmetric Accretion.
    C.Ho, R.Taam, B.Fryxell, T.Matsuda, H.Koide and E.Shima,
    Mon. Not. R. astr. Soc., 238, No.4 (1989), 1447- 1464, (16)
  65. Inhomogeneous Wind Accretion - Comparison between 3D and 2D Computations,
    K.Sawada, T.Matsuda, U.Anzer, G.Boerner and M.Livio,
    Astron. Astrophys., 221, No.2 (1989), 263-272, (29)
  66. Nonlinear Growth of Rayleigh-Taylor Instabilities and Mixing in SN1987A.
    I.Hachisu, T.Matsuda, K.Nomoto and T.Shigeyama,
    Astro. Phys. Lett., 358, No.2 (1990), L57-L61, (78)
  67. Mass Transfer by Tidally Induced Spiral Shocks in an accretion Disk.
    T.Matsuda, N.Sekino, K.Sawada, E.Shima and H.Spruit,
    Astron. Astrophys., 235, No.1/2 (1990), 211-218, (28)
  68. Instability of Astrophysical Jets. I --Numerical Simulation of Axisymmetric Opposing Jets--
    T.Matsuda, R.Ishii, Y.Umeda, A.Yasuda, K.Sawada and E.Shima,
    Prog. Theor. Phys., 84, No.5 (1990) Nov. 25, 837-855, (2)
  69. Instability of Astrophysical Jets. II --Numerical Simulation of Two-dimensional Choked Underexpanded Slab Jets--
    Y.Umeda, R.Ishii, T.Matsuda, A.Yasuda, K.Sawada and E.Shima,
    Prog. Theor. Phys., 84, No.5 (1990) Nov. 25, 856-866, (5)
  70. Rayleigh-Taylor Instabilities and Mixing in the Helium Star Models for Type Ib/Ic Supernovae.
    I.Hachisu, T.Matsuda, K.Nomoto and T.Shigeyama,
    Astro. Phys. Lett., 368, No.2 (1991), L27-L30, (59)
  71. On the Stability of Wind Accretion.
    T.Matsuda, N.Sekino, K.Sawada, E.Shima, M.Livio, U.Anzer and G.Boerner,
    Astron. Astrophys., 248, No.1 (1991), 301-314, (49)
  72. Numerical Simulations of Axisymmetric Accretion Flows.
    H.Koide, T.Matsuda and E.Shima,
    Mon. Not. R. astr. Soc., 252, No.4 (1991) 473-481, (16)
  73. On the "Flip-Flop" Instability of Bondi-Hoyle Accretion Flows.
    M.Livio, N.Soker, T.Matsuda and U.Anzer,
    Mon. Not. R. astr. Soc., 253, No.4 (1991) ,633-636, (24)
  74. Three-dimensional Hydrodynamic Simulation of an Accretion Flow in a Close Binary System.
    K.Sawada and T.Matsuda,
    Mon. Not. R. astr. Soc., 255, No.1 (1992), 17-20, (32)
  75. Numerical Simulations of Two-dimensional and Three- dimensional Accretion Flows.
    T.Matsuda, T.Ishii, N.Sekino, K.Sawada, E.Shima, M.Livio and U.Anzer,
    Mon. Not. R. astr. Soc., 255, No.2 (1992), 183-191, (30)
  76. Mixing in Ejecta of Supernovae I. General Properties of 2D Rayleigh-Taylor Instabilities.
    I.Hachisu, T.Matsuda, K.Nomoto and T.Shigeyama, Astrophys. J., 390, No.1 (1992), 230-252, (29)
  77. Spiral Shocks and Sub-day Variability in SS433
    S.K. Chakrabarti and T.Matsuda,
    Astrophys. J., 390 No.2 (1992), 639-644, (8)
  78. Hydrodynamics of Wind Accretion in Astrophysics.
    T.Matsuda, T.Ishii, N.Sekino, H.Koide, K.Sawada and E.Shima,
    Comp. Fluid Dynamics J., 1, No.262 (1992) 115-127.
  79. Numerical Simulations of Two-dimensional and Three-dimensional Wind Accretion Flows of an Isothermal Gas.
    T.Ishii, T.Matsuda, E.Shima, M.Livio, U.Anzer, G.Boerner,
    Astrophys. J., 404 No.2 (1993) 706-716, (30)
  80. Mixing in ejecta of supernovae. II. Mixing width of 2D Rayleigh-Taylor instabilities in the helium star models for type Ib/Ic supernovae.
    I.Hachisu, T.Matsuda, K.Nomoto and T.Shigeyama,
    Astron. & Astrophys. Suppl. Ser., 103, (1994) 341-364, (18)
  81. Spiral Shocks in Three-dimensional Accretion Discs.
    H.Yukawa, H.Boffin and T.Matsuda,
    Mon. N. R. astr. Soc., 292, (1997) 321-330, (28)
  82. Influence of the interstellar magnetic field direction on the shape of the global heliopause.
    N. Pogorelov and T.Matsuda,
    Journal of Geophysical Resaerch, 103, (1998) 237-245, (18)
  83. Numerical computation of two dimensional wind accretion of isothermal gas.
    E.Shima, T.Matsuda, U.Anzer, G.Boerner, H.Boffin,
    Astron. & Astrophys. 337 (1998) 311-320, (10)
  84. Effect of Radiation Drag on Hoyle-Lyttleton Accretion.
    T.Nio, T.Matsuda, J.Fukue,
    Publ. Astron. Soc. Japan 50 (1998) 495-500, (6)
  85. Towards steady-state solutions for supersonic wind accretion on to gravitating objects.
    N.V.Pogorelov, Y.Ohsugi, T.Matsuda,
    M.N. 313 (2000) 198-208, (11)
  86. Nonevolutionary MHD shocks in the solar wind and interstellar medium interaction.
    N.V.Pogorelov, T.Matsuda,
    Astron. & Astrophys. 354 (2000) 697-702, (10)
  87. Two- and Three-Dimensional Numerical Simulations of Accretion Discs in a Close Binary System.
    Makoto Makita, Kenji Miyawaki, Takuya Matsuda,
    MN 316 (2000) 906-916, (25)
  88. Numerical Simulation of Accretion Discs in Close Binary Systems and Discovery of Spiral Shocks.
    T.Matsuda, M.Makita, H.Fujiwara, T.Nagae, K.Haraguchi, E.Hayashi and H.Boffin
    Astrophys. Space Sci. 274 (2000), 259-273, (10)
  89. Is angular momentum in an accretion disk transported inwards?
    E.Hayashi and T.Matsuda,
    Progress of Theoretical Physics 105 (2001), 531-536, (3)
  90. Numerical simulation of interaction between an L1 stream and an accretion disk in a close binary system
    H.Fujiwara, M.Makita, T.Nagae and T.Matsuda
    Progress of Theoretical Physics 106 (2001),729-749, (2)
  91. Numerical simulation of the surface flow of a companion star in a close binary system
    K.Oka, T.Nagae, T.Matsuda, H.Fujiwara and H.M.J.Boffin
    Astron. & Astrophys. 394 (2002) 115-124 (5)
  92. Comment on "On the interaction of the solar wind with the interstellar medium: Field aligned MHD flow" by R. Ratkiewicz and G.M. Webb
    N. Pogorelov and T.Matsuda
    Journal Geophys. Res. 109 (2004) A02110
  93. Numerical Simulation of the Surface Flow on the Companion Star in a Close Binary System
    II. Construction of Doppler maps and application to Galactic supersoft X-ray sources
    K.Oka, T.Matsuda, I. Hachisu and H.M.J.Boffin
    Astron. & Astrophys 419 (2004) 277-283
  94. Wind Accretion in Binary Stars
    I. Mass accretion ratio
    T.Nagae, K.Oka, T.Matsuda, H.Fujiwara, I.Hachisu and H.M.J.Boffin
    Astron. & Astrophys. 419 (2004) 335-343 (5)
  95. The Structure of Cool Accretion Disc in Semidetached Binaries
    D.V.Bisikalo, A.A.Boyarchuk, P.V.Kaygorodov, O.A.Kuznetsov and T.Matsuda
    Astronomy Reports 81 (2004) 494-502
  96. A Model of Superoutbursts in Binaries of SU Uma Type
    D.V.Bisikalo, A.A.Boyarchuk, P.V.Kaygorodov, O.A.Kuznetsov and T.Matsuda
    Astronomy Reports 81 (2004) 648-657 (1)
  97. A Paradox of Two Space Ships in Special Relativity
    T. Matsuda and A. Kinoshita
    AAPPS Bulletin 14 (2004) 3-7 (3)
  98. On Kinetic Theory Viscosity in Rotating Gas
    T. Matsuda and E. Hayashi
    Progress of Theoretical Physics 112 (2004), 357-362
  99. Comments on "Angular Momentum Transport in Quasi-Keplerian Accretion Disks"
    E.Hayashi, H.Isaka and T.Matsuda
    Progress of Theoretical Physics 113 (2005) 1183-1191
  100. Wind accretion in binary stars.
    II Angular momentum loss
    B. Jahanara, M. Mitsumoto, K. Oka, T. Matsuda, I. Hachisu and H. Boffin
    Astron. & Astrophys 441 (2005) 589-595
  101. Three-Dimensional Gas-Dynamical Modeling of Changes in the Flow Structure during the Transition from the Quiescent to the Active State in Symbiotic Stars
    M.Mitsumoto, B.Jahanara, T.Matsuda, K.Oka, D.V.Bisikalo, E.Yu.Kilpio, H.M.J.Boffin, A.A.Boyarchuk, O.A.Kuznetsov
    Astronomy Reports 49 (2005) 884-891

    Proceedings, books and non-refereed papers
    1. On the Importance of the Thermal Boundary Condition to the Flow in a Strongly Rotating Fluid.
      T.Matsuda,
      Proc. 2nd Workshop on 'Gases in Strong Rotation' held at Cadarache, ed. Soubbaramayer (1977), 77-122.
    2. Meridional Flow of Compressible Fluid in a Rapidly Rotating Short Cylinder.
      K.Hashimoto and T.Matsuda,
      Proc. 3rd Workshop on 'Gases in Strong Rotation' held at Roma, ed. G.B.Scricini (1979), 103-128.
    3. Two Theoretical Ideas on the Large-Scale Distribution of Interstellar Matter.
      A.H.Nelson and T.Matsuda,
      in 'Giant Molecular Clouds in the Galaxy' ed. P.M.Solomon and M.G.Edmunds, Pergamon Press, Oxford (1980), 141-146.
    4. Non-Linear Corrugation Waves in Disk Galaxies.
      A.H.nelson and T.Matsuda
      PHOTOMETRY KINEMATICS AND DYN. OF GALAXIES 1980 (1980), 415.
    5. Non Axisymmetric Flow in a Rotating Cylinder.
      T.Matsuda, K.Nakagawa and H.Takeda,
      Proc. 4th Workshop on 'Gases in Strong Rotation' held at Oxford, ed. E.R\"atz (1981), 65-93.
    6. Atmospheric Circulation in a Space Colony. T.Matsuda,
      Solar Terestrial Environment Research (1983).
    7. Gas Flow in a Close Binary Star System.
      T.Matsuda, K.Sawada and I.Hachisu,
      Proc. 6th Workshop on 'Gases in Strong Rotation' held at Tokyo, ed. Takashima (1985).
    8. Numerical Simulation of Axisymmetric Accretion Flow on to a Compact Object.
      T.Matsuda, H.Koide, N.Sekino, K.Sawada and E.Shima,
      Proceedings of the international conference on "The Physics of Neutron Stars and Blackholes" held at Tokyo, ed. by Y. Tanaka (1988), University Academy Press, Tokyo, pp. 219-222.
    9. Numerical Simulation of Astrophysical Jets.
      T.Matsuda, R.Ishii, Y.Umeda, A.Yasuda, K.Sawada and E.Shima,
      in "Big Bang, Active Galactic Nuclei and Supernova", ed. by S. Hayakawa & K. Sato (1989), University Academy Press, Tokyo, pp. 337-338.
    10. Numerical Simulations of Cosmic Gas Dynamics and their Visulalization --Accretion Flow in a Close Binary Star System--
      T.Matsuda, N.Sekino, K.Sawada & E.Shima,
      presented at International Symposium on Computational Fluid Dynamics-Nagoya, August 28-31, (1989).
    11. Mass transfer by tidally induced spiral shocks in an accretion disc
      T.Matsuda, N.Sekino, E.Shima, K.Sawada and H.C.Spruit
      in "Theory of accretion disks, NATO ASI Series C." , Kluwer academic publishers. vol.290, pp.355-371 (1989)
    12. Interaction between Solar Wind and Magnetized Local Interstellar Medium.
      T.Matsuda and Y.Fujimoto,
      Proceedings of the 4th International School for Space Simulation, Nara, April 2-6, (1991).
    13. Flip-flop Instability of Wind-fed Accretion Flow.
      T.Matsuda, T.Ishii, M.Livio, U.Anzer and G.Boerner,
      presented at The 28th Yamada Conference on Frontiers of X-ray Astronomy, Nagoya, April 8-12, (1991).
    14. Three-dimensional Hydrodynamic Calculation of an Accretion Disc by SPH Scheme.
      M.Nagasawa and T.Matsuda,
      presented at The 28th Yamada Conference on Frontiers of X-ray Astronomy, Nagoya, April 8-12, (1991).
    15. Three-Dimensional Numerical Simulation of Accretion Discs
      K.Sawada and T.Matsuda
      Structure and Emission Properties of Accretion Disks, Proceedings of IAU Colloq. 129, the 6th Institute d'Astrophysique de Paris (IAP) Meeting, held in Paris, France, 2-6 July, 1990. Edited by C. Bertout, S. Collin-Souffrin, and J. P. Lasota. Gif-sur-Yvette: Editions Frontieres, (1991)., p.481
    16. Models for Type Ib/Ic Supernovae and SN 1987A: Nucleosynthesis, Mixing and Light Curves
      K.Nomoto, T.Shigeyama, S.Kumagai, I.Hachisu and T.Matsuda
      Supernova 1987A and other supernovae, ESO Conference and Workshop Proceedings, Proceedings of an ESO/EIPC Workshop, Marciana Marina, Isola d'Elba, September 17-22, 1990, Garching: European Southern Observatory (ESO), |c1991, edited by I. J. Danziger, and Kurt Kj&aauml;r., p.173
    17. Three-dimensional Hydrodynamic Calculation of an Accretion Disc by a Finite Volume Scheme.
      presented at The 28th Yamada Conference on Frontiers of X-ray Astronomy, Nagoya, April 8-12, (1991).
    18. Application of numerical methods to modeling the stellar wind and interstellar medium interaction.
      N.Pogorelov and T.Matsuda,
      Computational Fluid Dynamics Review 1998, World Scientific, Singapore. 2, (1998) 932-962
    19. Impact of nonstationaryity and magnetization on the solar wind and interstellar medium interaction.
      N.V.Pogorelov, T.Matsuda,
      EOS Transactions, 79 (1998) 707-708.
    20. Spiral Structure in IP Peg: Confronting Theory and Observation.
      T. Matsuda, M. Makita, H. Yukawa, H. M.J. Boffin,
      Proceedings of Numerical Astrophysics 1998, Tokyo, Japan, 10-13 March, 1998, eds. S. M. Miyama, K. Tomisaka and T. Hanawa (Kluwer Academic Publishers), (1999) 207-209.
    21. 3D Finite Volume Simulation of Accretion Discs with Spiral Shocks.
      M. Makita, T. Matsuda,
      Proceedings of Numerical Astrophysics 1998, Tokyo, Japan, 10-13 March, 1998, eds. S. M. Miyama, K. Tomisaka and T. Hanawa (Kluwer Academic Publishers), (1999) 227-228.
    22. Numerical Computation of Two Dimensional Wind Accretion of Isothermal Gas.
      E.Shima, T.Matsuda, U.Anzer, G.Borner, H.M.J. Boffin,
      Proceedings of Numerical Astrophysics 1998, Tokyo, Japan, 10-13 March, 1998, eds. S. M. Miyama, K. Tomisaka and T. Hanawa (Kluwer Academic Publishers), (1999) 225-226.
    23. Three-dimensional SPH simulations of accretion discs.
      H.M.J. Boffin, K.Haraguchi, T.Matsuda,
      "Disk instabilities in close binary systems - 25 years of the disk instability model", S. Mineshige and J.C. Wheeler, eds., Universal Academy Press, (1999) 137-142.
    24. 3D simulations of the spiral structure.
      T.Matsuda, M.Makita, H.M.J.Boffin,
      "Disk instabilities in close binary systems - 25 years of the disk instability model", S. Mineshige and J.C. Wheeler, eds., Universal Academy Press, (1999) 129-136.
    25. Spiral shocks in accretion discs: comparing models with observations.
      M.Makita, H.Yukawa, T.Matsuda, H.M.J.Boffin,
      "Disk instabilities in close binary systems - 25 years of the disk instability model", S. Mineshige and J.C. Wheeler, eds., Universal Academy Press, (1999) 147-150.
    26. Stationary solution for the supersonic wind accretion.
      Y.Ohsugi, T.Matsuda, N.V.Pogorelov,
      Star Formation 1999, Proceedings of Star Formation 1999, held in Nagoya, Japan, June 21-25, 1999, ed. T,Nakamoto, (1999) 407-408.
    27. Spiral shocks in accretion discs.
      K.Haraguchi, H.M.J.Boffin, T.Matsuda,
      Star Formation 1999, Proceedings of Star Formation 1999, held in Nagoya, Japan, June 21-25, 1999, ed. T,Nakamoto, (1999) 241-242.
    28. The mechanism of the optical variability of supersoft X-ray sources.
      A.Koyama, T.Matsuda, J.Fukue,
      Star Formation 1999, Proceedings of Star Formation 1999, held in Nagoya, Japan, June 21-25, 1999, ed. T,Nakamoto, (1999) 237-238.
    29. Direct Monte Carlo simulation of accretion disc.
      T.Matsuda, H.Mizutani, H.Boffin.
      "The Physics of Cataclismic Variables and Related Objects 2001" held in Goettingen, Germany, August 6-10, (2001)
    30. Application of DSMC method to astrophysical flows.
      T.Matsuda, H.Mizutani, H.Boffin.
      IAU Symposium 208 "Astrophysical Supercomputing using Particle Simulations"
      held in Tokyo, Japan, July 10-13, (2001)
    31. Numerical Simulation of the Surface Flow of a Companion Star in a
      semi-detached Binary System,
      K. Oka, T. Nagae, T. Matsuda, H. Fujiwara, & H. M. J. Boffin
      The Proceedings of the IAU 8th Asian-Pacific Regional Meeting, Volume II,
      Edited by S. Ikeuchi, J. Hearnshaw, and T. Hanawa, the Astronomical Society
      of Japan, (2002) 453-454
    32. Gas flow in close binary star systems
      T.Matsuda, K.Oka, I.Hachisu and H.M.J.Boffin,
      Proceedings of The 6th International Nobeyama Work shop on the New Century of Computational Fluid Dynamics, Nobeyama, Japan, April (2003)
    33. Numerical Simulation of the Surface Flow of a Companion Star in a Semi-detached Binary System and its Application to the Galactic Supersoft X-ray sources
      K. Oka, T. Matsuda, I. Hachisu, H. Boffin
      IAU Colloquim 194 "Compact Binaries in the Galaxy and beyond"
      La Paz, Baja California Sur, Mexico, November (2003)


    36. Memoires of the Faculty of Engineering of Kyoto University
    37. Comparison of Various Numerical Techniques in Gas Dynamics.
      H.Shigefuji and T.Matsuda,
      Memoires of the Faculty of Engineering, Kyoto Univ., 46, No.4 (1984).
    38. The Osher Upwind Scheme and its Application to Cosmic Gas Dynamics. K.Sawada, E.Shima, T.Matsuda and T.Inaguchi,
      Memoires of the Faculty of Engineering, Kyoto Univ., 48, No.2 (1986) May 17, 240-264.
    39. Numerical and Experimental Studies on Choked Underexpanded Jets.
      R.Ishii, T.Matsuda, Y.Umeda, A.Yasuda and K.Sawada,
      Mem. Fac. Eng. kyoto Univ., 49, No.1 (1987) Feb. 28, 84-110; AIAA paper 87-1378 (1987).
    40. A TVD scheme using Roe's flux and the ambient boundary condition.
      K.Sawada, E.Shima and T.Matsuda,
      Mem. Fac. Eng. Kyoto Univ., 51, No.2 (1989) April 30, 124-134.
    41. Numerical Simulations of Axisymmetric Flows in Astrophysics and their Visualization by a Video Movie.
      T.Matsuda, H.Koide, Y.Fujimoto, N,Sekino, K.Sawada and E.Shima,
      Mem. Fac. Eng. Kyoto Univ., 51, No.3 (1989) July 30, 198-205.

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