Zobrazeno 1 - 10
of 2 244
pro vyhledávání: '"UMEMOTO, T."'
Autor:
Akashi N, Umemoto T, Yamada H, Fujiwara T, Yamamoto K, Taniguchi Y, Sakakura K, Wada H, Momomura SI, Fujita H
Publikováno v:
Diabetes, Metabolic Syndrome and Obesity, Vol Volume 16, Pp 1043-1054 (2023)
Naoyuki Akashi,1 Tomio Umemoto,1 Hodaka Yamada,2 Takayuki Fujiwara,3 Kei Yamamoto,1 Yousuke Taniguchi,1 Kenichi Sakakura,1 Hiroshi Wada,1 Shin-ichi Momomura,1 Hideo Fujita1 1Division of Cardiovascular Medicine, Jichi Medical University Saitama Medica
Externí odkaz:
https://doaj.org/article/309ee3f6d99f438897e285be8a9d6247
Autor:
Eden, D. J., Moore, T. J. T., Currie, M. J., Rigby, A. J., Rosolowsky, E., Su, Y., Kim, Kee-Tae, Parsons, H., Morata, O., Chen, H. -R., Minamidani, T., Park, Geumsook, Ragan, S. E., Urquhart, J. S., Rani, R., Tahani, K., Billington, S. J., Deb, S., Figura, C., Fujiyoshi, T., Joncas, G., Liao, L. W., Liu, T., Ma, H., Tuan-Anh, P., Yun, Hyeong-Sik, Zhang, S., Zhu, M., Henshaw, J. D., Longmore, S. N., Kobayashi, M. I. N., Thompson, M. A., Ao, Y., Campbell-White, J., Ching, T. -C., Chung, E. J., Duarte-Cabral, A., Fich, M., Gao, Y., Graves, S. F., Jiang, X. -J., Kemper, F., Kuan, Y. -J., Kwon, W., Lee, C. W., Lee, J. -E., Liu, M., Penaloza, C. H., Peretto, N., Phuong, N. T., Pineda, J. E., Plume, R., Puspitaningrum, E., Samal, M. R., Soam, A., Sun, Y., Tang, X. D., Traficante, A., White, G. J., Yan, C. -H., Yang, A., Yuan, J., Yue, N., Bemis, A., Brunt, C. M., Chen, Z., Cho, J., Clark, P. C., Cyganowski, C. J., Friberg, P., Fuller, G. A., Han, I., Hoare, M. G., Izumi, N., Kim, H. -J., Kim, J., Kim, S., Koch, E. W., Kuno, N., Lacialle, K. M., Lai, S. -P., Lee, H. Lee Y. -H., Li, D. L., Liu, S. -Y., Mairs, S., Oka, T., Pan, Z., Qian, L., Scicluna, P., Shi, C. -S., Shi, H., Srinivasan, S., Tan, Q. -H., Thomas, H. S., Torii, K., Trejo, A., Umemoto, T., Violino, G., Wallstrom, S., Wang, B., Wu, Y., Yuan, L., Zhang, C., Zhang, M., Zhou, C., Zhou, J. J.
The latest generation of Galactic-plane surveys is enhancing our ability to study the effects of galactic environment upon the process of star formation. We present the first data from CO Heterodyne Inner Milky Way Plane Survey 2 (CHIMPS2). CHIMPS2 i
Externí odkaz:
http://arxiv.org/abs/2009.05073
Autor:
Sofue, Y., Kohno, M., Torii, K., Umemoto, T., Kuno, N., Tachihara, K., Minamidani, T., Fujita, S., Matsuo, M., Nishimura, A., Tsuda, Y., Seta, M.
The FUGIN CO survey with the Nobeyama 45-m Telescope revealed the 3D structure of a galactic shock wave in the tangential direction of the 4-kpc molecular arm. The shock front is located at G30.5+00.0+95 km/s on the up-stream (lower longitude) side o
Externí odkaz:
http://arxiv.org/abs/1807.06232
Discovery of molecular and atomic clouds associated with the gamma-ray supernova remnant Kesteven 79
Autor:
Kuriki, M., Sano, H., Kuno, N., Seta, M., Yamane, Y., Inaba, T., Nagaya, T., Yoshiike, S., Okawa, K., Tsutsumi, D., Hattori, Y., Kohno, M., Fujita, S., Nishimura, A., Ohama, A., Matsuo, M., Tsuda, Y., Torii, K., Minamidani, T., Umemoto, T., Rowell, G., Bamba, A., Tachihara, K., Fukui, Y.
We carried out $^{12}$CO($J$ = 1-0) observations of the Galactic gamma-ray supernova remnant (SNR) Kesteven 79 using the Nobeyama Radio Observatory 45 m radio telescope, which has an angular resolution of $\sim20$ arcsec. We identified molecular and
Externí odkaz:
http://arxiv.org/abs/1711.08165
Autor:
Yamagishi, M., Kaneda, H., Ishihara, D., Oyabu, S., Suzuki, T., Onaka, T., Nagayama, T., Umemoto, T., Minamidani, T., Nishimura, A., Matsuo, M., Fujita, S., Tsuda, Y., Kohno, M., Ohashi, S.
We present $Spitzer$/IRS mid-infrared spectral maps of the Galactic star-forming region M17 as well as IRSF/SIRIUS Br$\gamma$ and Nobeyama 45-m/FOREST $^{13}$CO ($J$=1--0) maps. The spectra show prominent features due to polycyclic aromatic hydrocarb
Externí odkaz:
http://arxiv.org/abs/1607.03622
Publikováno v:
Publ.Astron.Soc.Japan 60 (2008) 407-419
The ``integral-shaped filament'' of the Orion A giant molecular cloud was mapped in N2H+, and its northern end, the OMC-2/3 region was observed also in HC3N and CCS. The N2H+ distribution is similar to the dust continuum distribution, except for the
Externí odkaz:
http://arxiv.org/abs/0804.0111
Autor:
Tsuboi, M., Tosaki, T., Kuno, N., Nakanishi, K., Sawada, T., Umemoto, T., Trushkin, S. A., Kotani, T., Kawai, N., Kurono, Y., Handa, T., Kohno, K., Tsukagoshi, T., Kameya, O., Kobayashi, H., Fujisawa, K., Doi, A., Omodaka, T., Takaba, H., Sudou, H., Wakamatsu, K., Koyama, Y., Kawai, E., Mochizuki, N., Murata, Y.
We present the results of the multi-frequency observations of radio outburst of the microquasar Cyg X-3 in February and March 2006 with the Nobeyama 45-m telescope, the Nobeyama Millimeter Array, and the Yamaguchi 32-m telescope. Since the prediction
Externí odkaz:
http://arxiv.org/abs/0710.2722
Context. Molecular clouds near the H II regions tend to harbor more luminous protostars. Aims. Our aim in this paper is to investigate whether or not radiation-driven implosion mechanism enhances luminosity of protostars near regions of high-ionizing
Externí odkaz:
http://arxiv.org/abs/astro-ph/0702332
Autor:
Hirabayashi, H., Murata, Y., Edwards, P. G., Asaki, Y., Mochizuki, N., Inoue, M., Umemoto, T., Kameno, S., Kono, Y.
A second generation near-term space VLBI mission, VSOP-2, is being planned for a launch in 2010 or soon after. The scientific objectives are very high angular resolution imaging of astrophysically exotic regions, including the cores, jets, and accret
Externí odkaz:
http://arxiv.org/abs/astro-ph/0501020
Publikováno v:
Astrophys.J. 606 (2004) 333-340
N2H+ observations of molecular cloud cores in Taurus with the Nobeyama 45 m radio telescope are reported. We compare ``cores with young stars'' with ``cores without young stars''. The differences in core radius, linewidth, and core mass are small. Li
Externí odkaz:
http://arxiv.org/abs/astro-ph/0401584