Taniguchi, Y., & Murayama, T. (1998). Dusty tori of Seyfert nuclei probed by the water vapor
maser emission. How large are the dusty tori? Astrophysical Journal, 501, L25–L28.
Tatematsu, K., & Umemoto, T. (1991). Molecular cloud cores in the Orion A cloud. Societá
Astronomica Italiana, Memorie, 62(4), 813–821.
Tatematsu, K., Umemoto, T., et al. (1993). Molecular cloud cores in the Orion A
Cloud. I. Nobeyama CS (1-0). Astrophysical Journal, 404, 643–662.
Tomimatsu, A., & Sato, H. (1973). New metric of exact solution for gravitational fields of spinning
masses. Progress of Theoretical Physics, 50(1), 95–110.
Tomita, K. (1991). Reminis cences of Prof. Nariai Hidekazu. Astronomical Herald, 84, 93–96. (天
文月報, 冨田憲二: 成相秀一先生を偲 ぶ).
Tsuboi, M., Kawabata, T., et al. (1995). Galactic center arc -polarized plumes complex at 43 GHz.
Publications of the Astronomical Society of Japan, 47, 829–836.
Uchida, Y., & Shibata, K. (1985). Magneto dynamical acceleration of CO and optical bipolar flows
from the region of star formation. Publications of the Astronomical Society of Japan, 37,
515–535.
Uchida, Y., Sofue, Y., & Shibata, K. (1985). Origin of the galactic center lobes. Nature, 317, 699.
Uchida, Y., Kaifu, N., et al. (1987). Observations of the detailed structure and velocity field in the
CO bipolar flows associated with L1551 IRS-5. Publications of the Astronomical Society of
Japan, 39, 907–924.
Uchida, Y., Shibata, K., & Matsumoto, R. (1990). Magnetohydrodynamical simulation in
astrophysics – Jets, loops, and flares. Astronomical Herald, 83(6), 181–184. (天文月報, 内田
豊ほか: 天体の電磁流体現象のシミュレーション).
Unno, W. (1950). On the radiation pressure in a planetary nebula. I. Publications of the Astronomical Society of Japan, 2, 53–55.
Unno, W. (1952). On the radiation pressure in a planetary nebula. II. The problem of HeII.
Publications of the Astronomical Society of Japan, 3, 178–183.
Unno, W. (1956). Line formation of a normal Zeeman triplet. Publications of the Astronomical
Society of Japan, 8, 108–125.
Unno, W. (1971). Physical state and stability of super-massive objects. Publications of the
Astronomical Society of Japan, 23, 123–147.
Unno, W., & Kawabata, K. (1955). On the acoustic noise in the solar atmosphere. Publications of
the Astronomical Society of Japan, 7, 21–26.
Unno, W., & Takakubo, K. (1952). On the internal motions in planetary nebulae. Publications of
the Astronomical Society of Japan, 3, 195–208.
Unno, W., Osaki, Y., et al. (1979). Nonradial oscillations of stars. University of Tokyo Press.
Watanabe, T. (1988). An indication of extended chromosphere in line width – Luminosity relations.
Publications of the Astronomical Society of Japan, 40, 475–490.
Watanabe, Y., Inagaki, S., et al. (1981). Vlasov simulations of stellar disks. I. Axisymmetric case.
Publications of the Astronomical Society of Japan, 33, 541–565.
Yamaguchi, S., Kawada, M., et al. (1990). Optically thin hot plasma near the galactic center:
Mapping observations of the 6.7 KeV iron line. Astrophysical Journal, 365, 532–538.
Yamashita, Y., & Maehara, H. (1978a). The spectrum of the companion of Mira Ceti. Publications
of the Astronomical Society of Japan, 29, 319–329.
Yamashita, Y., & Maehara, H. (1978b). Mass loss from Mira Ceti. Publications of the Astronomical
Society of Japan, 30, 409–417.
Yokoyama, T., & Shibata, K. (1994). What is the condition for fast magnetic reconnection?
Astrophysical Journal, 436, L194–L200.
Yokoyama, T., & Shibata, K. (1998). A two-dimensional MHD simulation of chromospheric
evaporation in a solar flare based on a magnetic reconnection model. Astrophysical Journal,
494, L113–L116.
Yoshida, A., & Murakami, T. (1990). Cyclotron absorption features in γ-ray bursts and related
magnetic fields of neutron stars. Astronomical Herald, 83, 38–42. (天文月報, 吉田篤正, 村上
敏夫: γ線バーストのサイクロトロン吸収線と中性子星磁場).
References
247
maser emission. How large are the dusty tori? Astrophysical Journal, 501, L25–L28.
Tatematsu, K., & Umemoto, T. (1991). Molecular cloud cores in the Orion A cloud. Societá
Astronomica Italiana, Memorie, 62(4), 813–821.
Tatematsu, K., Umemoto, T., et al. (1993). Molecular cloud cores in the Orion A
Cloud. I. Nobeyama CS (1-0). Astrophysical Journal, 404, 643–662.
Tomimatsu, A., & Sato, H. (1973). New metric of exact solution for gravitational fields of spinning
masses. Progress of Theoretical Physics, 50(1), 95–110.
Tomita, K. (1991). Reminis cences of Prof. Nariai Hidekazu. Astronomical Herald, 84, 93–96. (天
文月報, 冨田憲二: 成相秀一先生を偲 ぶ).
Tsuboi, M., Kawabata, T., et al. (1995). Galactic center arc -polarized plumes complex at 43 GHz.
Publications of the Astronomical Society of Japan, 47, 829–836.
Uchida, Y., & Shibata, K. (1985). Magneto dynamical acceleration of CO and optical bipolar flows
from the region of star formation. Publications of the Astronomical Society of Japan, 37,
515–535.
Uchida, Y., Sofue, Y., & Shibata, K. (1985). Origin of the galactic center lobes. Nature, 317, 699.
Uchida, Y., Kaifu, N., et al. (1987). Observations of the detailed structure and velocity field in the
CO bipolar flows associated with L1551 IRS-5. Publications of the Astronomical Society of
Japan, 39, 907–924.
Uchida, Y., Shibata, K., & Matsumoto, R. (1990). Magnetohydrodynamical simulation in
astrophysics – Jets, loops, and flares. Astronomical Herald, 83(6), 181–184. (天文月報, 内田
豊ほか: 天体の電磁流体現象のシミュレーション).
Unno, W. (1950). On the radiation pressure in a planetary nebula. I. Publications of the Astronomical Society of Japan, 2, 53–55.
Unno, W. (1952). On the radiation pressure in a planetary nebula. II. The problem of HeII.
Publications of the Astronomical Society of Japan, 3, 178–183.
Unno, W. (1956). Line formation of a normal Zeeman triplet. Publications of the Astronomical
Society of Japan, 8, 108–125.
Unno, W. (1971). Physical state and stability of super-massive objects. Publications of the
Astronomical Society of Japan, 23, 123–147.
Unno, W., & Kawabata, K. (1955). On the acoustic noise in the solar atmosphere. Publications of
the Astronomical Society of Japan, 7, 21–26.
Unno, W., & Takakubo, K. (1952). On the internal motions in planetary nebulae. Publications of
the Astronomical Society of Japan, 3, 195–208.
Unno, W., Osaki, Y., et al. (1979). Nonradial oscillations of stars. University of Tokyo Press.
Watanabe, T. (1988). An indication of extended chromosphere in line width – Luminosity relations.
Publications of the Astronomical Society of Japan, 40, 475–490.
Watanabe, Y., Inagaki, S., et al. (1981). Vlasov simulations of stellar disks. I. Axisymmetric case.
Publications of the Astronomical Society of Japan, 33, 541–565.
Yamaguchi, S., Kawada, M., et al. (1990). Optically thin hot plasma near the galactic center:
Mapping observations of the 6.7 KeV iron line. Astrophysical Journal, 365, 532–538.
Yamashita, Y., & Maehara, H. (1978a). The spectrum of the companion of Mira Ceti. Publications
of the Astronomical Society of Japan, 29, 319–329.
Yamashita, Y., & Maehara, H. (1978b). Mass loss from Mira Ceti. Publications of the Astronomical
Society of Japan, 30, 409–417.
Yokoyama, T., & Shibata, K. (1994). What is the condition for fast magnetic reconnection?
Astrophysical Journal, 436, L194–L200.
Yokoyama, T., & Shibata, K. (1998). A two-dimensional MHD simulation of chromospheric
evaporation in a solar flare based on a magnetic reconnection model. Astrophysical Journal,
494, L113–L116.
Yoshida, A., & Murakami, T. (1990). Cyclotron absorption features in γ-ray bursts and related
magnetic fields of neutron stars. Astronomical Herald, 83, 38–42. (天文月報, 吉田篤正, 村上
敏夫: γ線バーストのサイクロトロン吸収線と中性子星磁場).
References
247