Zobrazeno 1 - 10
of 130
pro vyhledávání: '"Ozeki, Hiroyuki"'
We have carried out observations of CCH and its two $^{13}$C isotopologues, $^{13}$CCH and C$^{13}$CH, in the 84 - 88 GHz band toward two starless cores, L1521B and L134N (L183), using the Nobeyama 45 m radio telescope. We have detected C$^{13}$CH wi
Externí odkaz:
http://arxiv.org/abs/1908.09983
Autor:
Taniguchi, Kotomi, Miyamoto, Yusuke, Saito, Masao, Sanhueza, Patricio, Shimoikura, Tomomi, Dobashi, Kazuhito, Nakamura, Fumitaka, Ozeki, Hiroyuki
We have carried out interferometric observations of cyanopolyynes, HC$_{3}$N, HC$_{5}$N, and HC$_{7}$N, in the 36 GHz band toward the G28.28$-$0.36 high-mass star-forming region using the Karl G. Jansky Very Large Array (VLA) Ka-band receiver. The sp
Externí odkaz:
http://arxiv.org/abs/1808.08435
Autor:
Taniguchi, Kotomi, Saito, Masao, Majumdar, Liton, Shimoikura, Tomomi, Dobashi, Kazuhito, Ozeki, Hiroyuki, Nakamura, Fumitaka, Hirota, Tomoya, Minamidani, Tetsuhiro, Miyamoto, Yusuke, Kaneko, Hiroyuki
We have carried out observations in the 42$-$46 and 82$-$103 GHz bands with the Nobeyama 45-m radio telescope, and in the 338.2$-$339.2 and 348.45$-$349.45 GHz bands with the ASTE 10-m telescope toward three high-mass star-forming regions containing
Externí odkaz:
http://arxiv.org/abs/1804.05205
We observed the $J=5-4$ rotational lines of the normal species and three $^{13}$C isotopologues of HC$_{3}$N at the 45 GHz band toward two low-mass starless cores, L1521B and L134N (L183), using the Nobeyama 45 m radio telescope in order to study the
Externí odkaz:
http://arxiv.org/abs/1707.08267
Autor:
Taniguchi, Kotomi, Saito, Masao, Hirota, Tomoya, Ozeki, Hiroyuki, Miyamoto, Yusuke, Kaneko, Hiroyuki, Minamidani, Tetsuhiro, Shimoikura, Tomomi, Nakamura, Fumitaka, Dobashi, Kazuhito
We carried out line survey observations at the 26-30 GHz band toward the four high-mass star-forming regions containing hot cores, G10.30-0.15, G12.89+0.49, G16.86-2.16, and G28.28-0.36, with the Robert C. Byrd Green Bank Telescope. We have detected
Externí odkaz:
http://arxiv.org/abs/1706.02465
We observed the J=9-8 and 10-9 rotational lines of three13C isotopologues of HC3N in L1527 and G28.28-0.36 with the 45-m radio telescope of the Nobeyama Radio Observatory in order to constrain the main formation mechanisms of HC3N in each source. The
Externí odkaz:
http://arxiv.org/abs/1608.01702
Autor:
Taniguchi, Kotomi, Ozeki, Hiroyuki, Saito, Masao, Sakai, Nami, Nakamura, Fumitaka, Kameno, Seiji, Takano, Shuro, Yamamoto, Satoshi
Publikováno v:
The Astrophysical Journal, 817:147 (2016)
We observed the J = 9-8 and 16-15 rotational transitions of the normal species and five 13C isotopologues of HC5N to study its formation mechanisms toward the cyanopolyyne peak in Taurus Molecular Cloud-1, with the 45-m radio telescope of Nobeyama Ra
Externí odkaz:
http://arxiv.org/abs/1512.05783
Autor:
Ikeda, Masafumi, Maezawa, Hiroyuki, Ito, Tetsuya, Saito, Gaku, Sekimoto, Yutaro, Yamamoto, Satoshi, Tatematsu, Ken'ichi, Arikawa, Yuji, Aso, Yoshiyuki, Noguchi, Takashi, Shi, Sheng-Cai, Miyazawa, Keisuke, Saito, Syuji, Ozeki, Hiroyuki, Fujiwara, Hideo, Ohishi, Masatoshi, Inatani, Junji
Publikováno v:
ApJ. 527 (1999), L59
Large scale mapping observations of the 3P1-3P0 fine structure transition of atomic carbon (CI, 492 GHz) and the J=3-2 transition of CO (346 GHz) toward the Orion A molecular cloud have been carried out with the Mt. Fuji submillimeter-wave telescope.
Externí odkaz:
http://arxiv.org/abs/astro-ph/9912261
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