Hori, K., Yokoyama, T., et al. (1997). Pseudo-two-dimensional hydrodynamic modeling of solar
flare loops. Astrophysical Journal, 489, 426–441.
Hoshi, R. (1981). Theory of steady accretion disks. Progress of Theoretical Physics Supplement,
70, 181–201.
Hoshi, R. (1998). Hydrogen Shell burning models for RX J0925.7 – 4758. Publications of the
Astronomical Society of Japan, 50, 501–507.
Ichikawa, T., Nakano, M., et al. (1985). CO observations of a spiral arm in M 31. Publications of the
Astronomical Society of Japan, 37, 439–450.
Ichimaru, S. (1977). Bimodal behavior of accretion disks: Theory and application to Cygnus X-1
transitions. Astrophysical Journal, 214, 840–853.
Ishida, K., & Kawajiri, N. (1968). Absolute iso-photometry of Galactic H II regions in Hα light.
Publications of the Astronomical Society of Japan, 20, 95–120.
Ishida, M., Matsuzaki, K., et al. (1997). Detailed X-ray spectroscopy of AM Herculis with ASCA.
Monthly Notices of the Royal Astronomical Society, 287, 651–662.
Isobe, S. (1973). Dust, stars and hydrogen distribution in the Orion Association. IAU Symposium,
52, 433–445.
Kaifu, N., Iguchi, T., & Kato, T. (1974). Gaseous structure in the Galactic center region. Publications of the Astronomical Society of Japan, 26, 117–128.
Kaifu, N., Suzuki, S., et al. (1984). Rotating gas disk around L 1551 IRS-5. Astronomy and
Astrophysics, 134, 7–12.
Kakubari, K., Hoshi, R., et al. (1989). Thermal instability in optically-thick accretion disks and
emergent X-ray spectra. Publications of the Astronomical Society of Japan, 41, 1035–1048.
Kambe, E., & Osaki, Y. (1988). Line profile variation due to nonradial oscillations in rapidly
rotating stars. Publications of the Astronomical Society of Japan, 40, 313–329.
Kameya, O., & Takakubo, K. (1988). The interface between the NGC 7538 H II region and its
molecular cloud core. Publications of the Astronomical Society of Japan, 40, 413–420.
Kameya, O., Hasegawa, T., et al. (1989). High-velocity flows in the NGC 7538 molecular cloud.
Astrophysical Journal, 339, 222–230.
Karoji, H., & Kodaira, K. (1972). Extremely compact galaxy CGCG 1622+4112. Publications of
the Astronomical Society of Japan, 24, 239–246.
Katahira, J., Hirata, R., et al. (1996). Period analysis of the radial velocity in Pleione. Publications
of the Astronomical Society of Japan, 48, 317–334.
Kato, M. (1983). Neutron star wind. Publications of the Astronomical Society of Japan, 35, 33–48.
Kato, S. (2000). Transition from standard disk to advection-dominated accretion flow. Astrophysical Journal, 538, 295–308.
Kato, S., & Fukue, J. (1980). Trapped radial oscillations of gaseous disks around a black hole.
Publications of the Astronomical Society of Japan, 32, 377–388.
Kawajiri, N., & Akabane, K. (1967). A morphological study of galactic H II regions. Publications
of the Astronomical Society of Japan, 19, 476–487.
Kinoshita, H. (1978). Dynamics of planets and satellites and theories of their motion. In Proceedings of the forty-first Colloquium, Cambridge, England, August 17–19, 1976
(pp. 241–257). Dordrecht: D. Reidel Publishing Co.. Third-order solution of an artificialsatellite theory.
Kinoshita, H. (2018). Obituary, Professor Kozai and celestial mechanics. Astronomical Herald,
111(7) (天文月報, 木下宙: 古在先生と天体力学).
Kinoshita, H., & Hori, G. (1972). On the stationary solutions for the problem of artificial satellites.
Tokyo Astronomical Observatory Report, 16(60), 230–240. (木下宙, 堀源一郎: 人工衛星の
運動の定常解について).
Kitamura, M. (1954). The effect of reflection upon the reduction of mass from the observed
velocity-curved of close binary systems. Publications of the Astronomical Society of Japan, 6,
217–228.
242
7 Postwar Development of Astrophysics, 1946–2000 (Part II: Astrophysics)
flare loops. Astrophysical Journal, 489, 426–441.
Hoshi, R. (1981). Theory of steady accretion disks. Progress of Theoretical Physics Supplement,
70, 181–201.
Hoshi, R. (1998). Hydrogen Shell burning models for RX J0925.7 – 4758. Publications of the
Astronomical Society of Japan, 50, 501–507.
Ichikawa, T., Nakano, M., et al. (1985). CO observations of a spiral arm in M 31. Publications of the
Astronomical Society of Japan, 37, 439–450.
Ichimaru, S. (1977). Bimodal behavior of accretion disks: Theory and application to Cygnus X-1
transitions. Astrophysical Journal, 214, 840–853.
Ishida, K., & Kawajiri, N. (1968). Absolute iso-photometry of Galactic H II regions in Hα light.
Publications of the Astronomical Society of Japan, 20, 95–120.
Ishida, M., Matsuzaki, K., et al. (1997). Detailed X-ray spectroscopy of AM Herculis with ASCA.
Monthly Notices of the Royal Astronomical Society, 287, 651–662.
Isobe, S. (1973). Dust, stars and hydrogen distribution in the Orion Association. IAU Symposium,
52, 433–445.
Kaifu, N., Iguchi, T., & Kato, T. (1974). Gaseous structure in the Galactic center region. Publications of the Astronomical Society of Japan, 26, 117–128.
Kaifu, N., Suzuki, S., et al. (1984). Rotating gas disk around L 1551 IRS-5. Astronomy and
Astrophysics, 134, 7–12.
Kakubari, K., Hoshi, R., et al. (1989). Thermal instability in optically-thick accretion disks and
emergent X-ray spectra. Publications of the Astronomical Society of Japan, 41, 1035–1048.
Kambe, E., & Osaki, Y. (1988). Line profile variation due to nonradial oscillations in rapidly
rotating stars. Publications of the Astronomical Society of Japan, 40, 313–329.
Kameya, O., & Takakubo, K. (1988). The interface between the NGC 7538 H II region and its
molecular cloud core. Publications of the Astronomical Society of Japan, 40, 413–420.
Kameya, O., Hasegawa, T., et al. (1989). High-velocity flows in the NGC 7538 molecular cloud.
Astrophysical Journal, 339, 222–230.
Karoji, H., & Kodaira, K. (1972). Extremely compact galaxy CGCG 1622+4112. Publications of
the Astronomical Society of Japan, 24, 239–246.
Katahira, J., Hirata, R., et al. (1996). Period analysis of the radial velocity in Pleione. Publications
of the Astronomical Society of Japan, 48, 317–334.
Kato, M. (1983). Neutron star wind. Publications of the Astronomical Society of Japan, 35, 33–48.
Kato, S. (2000). Transition from standard disk to advection-dominated accretion flow. Astrophysical Journal, 538, 295–308.
Kato, S., & Fukue, J. (1980). Trapped radial oscillations of gaseous disks around a black hole.
Publications of the Astronomical Society of Japan, 32, 377–388.
Kawajiri, N., & Akabane, K. (1967). A morphological study of galactic H II regions. Publications
of the Astronomical Society of Japan, 19, 476–487.
Kinoshita, H. (1978). Dynamics of planets and satellites and theories of their motion. In Proceedings of the forty-first Colloquium, Cambridge, England, August 17–19, 1976
(pp. 241–257). Dordrecht: D. Reidel Publishing Co.. Third-order solution of an artificialsatellite theory.
Kinoshita, H. (2018). Obituary, Professor Kozai and celestial mechanics. Astronomical Herald,
111(7) (天文月報, 木下宙: 古在先生と天体力学).
Kinoshita, H., & Hori, G. (1972). On the stationary solutions for the problem of artificial satellites.
Tokyo Astronomical Observatory Report, 16(60), 230–240. (木下宙, 堀源一郎: 人工衛星の
運動の定常解について).
Kitamura, M. (1954). The effect of reflection upon the reduction of mass from the observed
velocity-curved of close binary systems. Publications of the Astronomical Society of Japan, 6,
217–228.
242
7 Postwar Development of Astrophysics, 1946–2000 (Part II: Astrophysics)