|
Sorai, K. |
Volume |
Paper Title |
Page Number |
Authors |
124 |
The CO 2-1/1-0 ratio in the southern Milky Way and the Large Magellanic Cloud |
244 |
Hasegawa, T.; Morino, J.; Sorai, K.; Handa, T.; Sato, K.; Oka, T.; Seta, M.; Sakamoto, S.; Hayashi, M.; Booth, R.; Nyman, L. K.; Bronfman, L.; Rubio, M.; Shaver, P. |
168 |
The Tokyo-Nobeyama CO J=2-1 Galactic Plane Survey |
90 |
Sakamoto, S.; Hasegawa, T.; Handa, T.; Morino, J.-I.; Oka, T.; Seta, M.; Sorai, K.; Usuda, K. S.; Hayashi, M. |
230 |
Distribution and Kinematics of Molecular Gas in NGC 3504 |
379 |
Kuno, N.; Nishiyama, K.; Nakai, N.; Sorai, K.; Vila-VilarĂ³, B.; Handa, T. |
230 |
HCN/CO Ratio in the Nuclear Regions and the Disks of Nearby Spiral Galaxies |
385 |
Sorai, K.; Nakai, N.; Kuno, N.; Nishiyama, K. |
476 |
High Gas Fraction of Barred Spiral Galaxies at z ∼ 0.1–0.2 |
277 |
Matsui, K.; Sorai, K.; Baba, J.; Watanabe, Y.; Kuno, N. |
476 |
New Detection of an Extremely Blue-shift Dominated Jet in G353.273+0.641: A Possible Disk-Jet System on 100 AU Scale |
381 |
Motogi, K.; Fujisawa, K.; Sugiyama, K.; Niinuma, K.; Sorai, K.; Honma, M.; Hirota, T.; Yonekura, Y.; Hachisuka, K.; Walsh, A. J. |
476 |
Development of 32-m Radio Telescopes for
Monitoring Observations of
Methanol Masers, H2O Masers, and Radio Continuum |
415 |
Yonekura, Y.; Saito, Y.; Saito, T.; Mori, T.; Soon, K. L.; Momose, M.; Yokosawa, M.; Ogawa, H.; Fujisawa, K.; Sugiyama, K.; Motogi, K.; Takaba, H.; Sorai, K.; Nakai, N.; Kameno, S.; Kobayashi, H.; Kawaguchi, N.; Hachisuka, K. |
499 |
Ionized Gas Observation Toward a Nearby Starburst Galaxy NGC 253 |
117 |
Nakanishi, K.; Sorai, K.; Nakai, N.; Kuno, N.; Matsubayashi, K.; Sugai, H.; Takano, S.; Kohno, K.; Nakajima, T. |
499 |
Spectral Line Survey Toward Spiral Arm of M51 |
151 |
Watanabe, Y.; Sakai, N.; Sorai, K.; Nishimura, Y.; Yamamoto, S. |
499 |
CO Emissions from Optically Selected Galaxies at z∼0.1–0.2: Tight Anti-Correlation Between Molecular Gas Fraction and 4000 Angstrom Break Strength |
157 |
Morokuma-Matsui, K.; Baba, J.; Sorai, K.; Kuno, N. |
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