Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Keita Hosaka"'
Autor:
Ryoko Yoshino, Tasuku Tabata, Kenji Date, Arata Okuyama, Masaya Takahashi, Keita Hosaka, Hidehiko Murata
Publikováno v:
Journal of the Meteorological Society of Japan. Ser. II. :91-109
Issue: Special Issue on Meteorology and Climate Change Studies by Using the Geostationary Meteorological Satellite Himawari-8
資料番号: SA1180176000
資料番号: SA1180176000
Autor:
Hidehiko Murata, Arata Okuyama, Keita Hosaka, Nobutaka Mori, Masaya Takahashi, Kotaro Bessho, Ryuichiro Nakayama, Kenji Date, Akiyoshi Andou, Ryo Dojo, Tasuku Tabata
Publikováno v:
SPIE Proceedings.
The new-generation Himawari-8 geostationary meteorological satellite of the Japan Meteorological Agency (JMA) started operation in July 2015 after the completion of in-orbit testing and checking of the overall system. Himawari-8 features the new Adva
Autor:
T. Takekoshi, Mareki Honma, Kazuhito Motogi, Yukie Ohishi, Yoshimasa Watanabe, Kazunori Akiyama, Kazuo Sorai, Keita Hosaka, Hiroshi Kobayashi, Asao Habe, Ken Tateuchi, Tetsuhiro Minamidani
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 417:238-249
We have performed VLBI and single-dish monitoring of 22 GHz H$_{2}$O maser emission from the high mass young stellar object G353.273+0.641 with VERA (VLBI Exploration of Radio Astrometry) and Tomakamai 11-m radio telescope. Two maser flares have been
Large-Scale NH3Observations toward the Galactic Star-Forming Regions I. W 51 Molecular Cloud Complex
Autor:
Sakurako Sumida, Yukie Ohishi, Moritaka Kimura, Masayuki Y. Fujimoto, Kazuhito Motogi, Shinichi Miwa, Hiroyuki Nishitani, Yasuhiro Koyama, Asao Habe, Yoshimasa Watanabe, Kazuo Sorai, Ryosuke Uchida, Tetsuhiro Minamidani, Naomasa Nakai, Noboru Kaneko, Yoshiaki Fukuya, Johta Awano, Keita Hosaka
Publikováno v:
Publications of the Astronomical Society of Japan. 60:1285-1296
Large-area observations of dense molecular gas were made in NH3 (J , K) = (1, 1), (2, 2), and (3, 3) inversion lines with 4: 0 5 resolution toward the molecular cloud complex of the W 51 region. The observations were a part of a NH3 survey of the Gal
Autor:
Tetsuhiro Minamidani, Yukie Ohishi, Keita Hosaka, Asao Habe, Masayuki Y. Fujimoto, Yoshimasa Watanabe, Kazuhito Motogi, Kazuo Sorai, Hiroyuki Nishitani
Publikováno v:
Publications of the Astronomical Society of Japan. 64:30
We consider the properties of giant molecular cloud complexes in the star-forming region W 43 with a resolution of several pc scale, and discuss their relations to the evolutionary stages of massive star formation. We performed aN H 3 (J , K) = (1, 1