Zobrazeno 1 - 7
of 7
pro vyhledávání: '"Takeru Murase"'
Autor:
Mikito Kohno, James O Chibueze, Ross A Burns, Toshihiro Omodaka, Toshihiro Handa, Takeru Murase, Rin I Yamada, Takumi Nagayama, Makoto Nakano, Kazuyoshi Sunada, Kengo Tachihara, Yasuo Fukui
Publikováno v:
Publications of the Astronomical Society of Japan. 75:397-415
We have carried out the NH$_3$ $(J,K)=(1,1),(2,2),$ and $(3,3)$ mapping observations toward the Galactic infrared bubble N49 (G28.83-0.25) using the Nobeyama 45 m telescope. Three NH$_3$ clumps (A, B, and C) were discovered along the molecular filame
Autor:
Takeru Murase, Toshihiro Handa, Ren Matsusaka, Yoshito Shimajiri, Masato I N Kobayashi, Mikito Kohno, Junya Nishi, Norimi Takeba, Yosuke Shibata
Publikováno v:
Monthly Notices of the Royal Astronomical Society.
We studied the H$_2$ column density probability distribution function (N-PDF) based on molecular emission lines using the Nobeyama 45-m Cygnus X CO survey data. Using the DENDROGRAM and SCIMES algorithms, we identified 124 molecular clouds in the $^{
Autor:
Mikito Kohno, Toshihiro Omodaka, Toshihiro Handa, James O Chibueze, Takumi Nagayama, Ross A Burns, Takeru Murase, Ren Matsusaka, Makoto Nakano, Kazuyoshi Sunada, Rin I Yamada, John H Bieging
Publikováno v:
Publications of the Astronomical Society of Japan. 74:545-556
We performed NH$_3\ (J,K)=(1,1),(2,2),$ and $(3,3)$ mapping observations toward the Galactic massive star-forming region Sh 2-255 and Sh 2-257 using the Nobeyama 45-m telescope as a part of the KAGONMA (KAgoshima Galactic Object survey with the Nobey
Autor:
Takeru Murase, Toshihiro Handa, Yushi Hirata, Toshihiro Omodaka, Makoto Nakano, Kazuyoshi Sunada, Yoshito Shimajiri, Junya Nishi
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2022, 510, pp.1106-1117. ⟨10.1093/mnras/stab3472⟩
Monthly Notices of the Royal Astronomical Society, 2022, 510, pp.1106-1117. ⟨10.1093/mnras/stab3472⟩
We present the results of NH3 (1,1), (2,2) and (3,3) and H2O maser simultaneous mapping observations toward the high-mass star-forming region W33 with the Nobeyama 45-m radio telescope. W33 has six dust clumps and one of which, W33 Main, is associate
Autor:
Yuuki Adachi, Makoto Shizugami, Yoshiaki Tamura, Syunsaku Suzuki, Nobuyuki Sakai, Daichi Kaseda, Takumi Nagayama, Shota Hamada, Koji Wada, Kazuyoshi Sunada, Jeong Sook Kim, Tomoharu Kurayama, Daichi Inenaga, Tomoya Hirota, Yuan Wei Wu, Hiroyuki Nakanishi, Miyako Oyadomari, Yuri Uno, Riku Urago, Yoshiaki Hagiwara, Chung Sik Oh, Kazuhiro Hada, Ken Takahashi, Atsushi Morita, Kazuya Hachisuka, Fumie Tazaki, Katsunori M. Shibata, Aya Yamauchi, Mao Hashimoto, Koichiro Sugiyama, Hideyuki Kobayashi, Yusuke Kono, Osamu Kameya, Tomoaki Oyama, Daisuke Sakai, Yoon Kyung Choi, Yuji Ueno, Masako Matsuno, Takaaki Jike, Jungha Kim, Toshihiro Omodaka, Kazuyoshi Yamashita, Takeru Murase, Yuto Yamashita, Ken Hirano, Kotaro Niinuma, Hiroshi Imai, Kazuhito Motogi, Toshio Ishikawa, Mareki Honma, Yushi Hirata, Junya Nishi, James O. Chibueze, Toshihiro Handa, Akiharu Nakagawa, Ross A. Burns, Mi Kyoung Kim, Jumpei Sudo, Takanori Ichikawa, Satoko Sawada-Satoh, Akito Yuda
We present the first astrometry catalog from the Japanese VLBI (very long baseline interferometer) project VERA (VLBI Exploration of Radio Astrometry). We have compiled all the astrometry results from VERA, providing accurate trigonometric annual par
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2ab763141284a86a61bdddacb90ad1c1
Autor:
K. Sunada, T. Minamidani, Shinji Fujita, Yuya Tsuda, M. Maebata, Nario Kuno, Makoto Nakano, Takeru Murase, K. Wada, Tomofumi Umemoto, Mika Kuriki, Z. Yang, Toshihiro Omodaka, Atsushi Nishimura, Yushi Hirata, Mitsuhiro Matsuo, K. Torii, K. Ishizaki, Toshihiro Handa, S. Shihara, M. Kohno
Publikováno v:
Proceedings of the International Astronomical Union. 14:353-354
In the collapsing phase of a molecular cloud, the molecular gas temperature is a key to understand the evolutionary process from a dense molecular cloud to stars. In order to know this, mapping observations in NH3 lines are required. Therefore, we ma
Autor:
Tomofumi Umemoto, Kazufumi Torii, Miru Maebata, Atsushi Nishimura, Yuya Tsuda, Takeru Murase, Mitsuhiro Matsuo, Toshihiro Handa, Mikito Kohno, Shinji Fujita, Mika Kuriki, Nario Kuno, Tetsuhiro Minamidani
Publikováno v:
Proceedings of the International Astronomical Union. 14:322-323
“Gas Density Histogram (GDH)” is an observational counterpart of the probability density function (PDF) of the gas density of interstellar medium (ISM). We used 12CO data in (l, b) = (29°, 0) region from “FOREST unbiased galactic imaging surve