Zobrazeno 1 - 10
of 320
pro vyhledávání: '"Kan YA"'
Autor:
Niinuma, Kotaro, Lee, Sang-Sung, Kino, Motoki, Sohn, Bong Won, Akiyama, Kazunori, Zhao, Guang-Yao, Sawada-Satoh, Satoko, Trippe, Sascha, Hada, Kazuhiro, Jung, Taehyun, Hagiwara, Yoshiaki, Dodson, Richard, Koyama, Shoko, Honma, Mareki, Nagai, Hiroshi, Chung, Aeree, Doi, Akihiro, Fujisawa, Kenta, Han, Myoung-Hee, Kim, Joeng-Sook, Lee, Jeewon, Lee, Jeong Ae, Miyazaki, Atsushi, Oyama, Tomoaki, Sorai, Kazuo, Wajima, Kiyoaki, Bae, Jaehan, Byun, Do-Young, Cho, Se-Hyung, Choi, Yoon Kyung, Chung, Hyunsoo, Chung, Moon-Hee, Han, Seog-Tae, Hirota, Tomoya, Hwang, Jung-Wook, Je, Do-Heung, Jike, Takaaki, Jung, Dong-Kyu, Jung, Jin-Seung, Kang, Ji-Hyun, Kang, Jiman, Kang, Yong-Woo, Kan-ya, Yukitoshi, Kanaguchi, Masahiro, Kawaguchi, Noriyuki, Kim, Bong Gyu, Kim, Hyo Ryoung, Kim, Hyun-Goo, Kim, Jaeheon, Kim, Jongsoo, Kim, Kee-Tae, Kim, Mikyoung, Kobayashi, Hideyuki, Kono, Yusuke, Kurayama, Tomoharu, Lee, Changhoon, Lee, Jung-Won, Lee, Sang Hyun, Minh, Young Chol, Matsumoto, Naoko, Nakagawa, Akiharu, Oh, Chung Sik, Oh, Se-Jin, Park, Sun-Youp, Roh, Duk-Gyoo, Sasao, Tetsuo, Shibata, Katsunori M., Song, Min-Gyu, Tamura, Yoshiaki, Wi, Seog-Oh, Yeom, Jae-Hwan, Yun, Young Joo
The Korean very-long-baseline interferometry (VLBI) network (KVN) and VLBI Exploration of Radio Astrometry (VERA) Array (KaVA) is the first international VLBI array dedicated to high-frequency (23 and 43 GHz bands) observations in East Asia. Here, we
Externí odkaz:
http://arxiv.org/abs/1406.4356
Autor:
Matsumoto, Naoko, Hirota, Tomoya, Sugiyama, Koichiro, Kim, Kee-Tae, Kim, Mikyoung, Byun, Do-Young, Jung, Taehyun, Chibueze, James O., Honma, Mareki, Kameya, Osamu, Kim, Jongsoo, Lyo, A-Ran, Motogi, Kazuhito, Oh, Chungsik, Shino, Nagisa, Sunada, Kazuyoshi, Bae, Jaehan, Chung, Hyunsoo, Chung, Moon-Hee, Cho, Se-Hyung, Han, Myoung-Hee, Han, Seog-Tae, Hwang, Jung-Wook, Je, Do-Heung, Jike, Takaaki, Jung, Dong-Kyu, Jung, Jin-seung, Kang, Ji-hyun, Kang, Jiman, Kang, Yong-Woo, Kan-ya, Yukitoshi, Kawaguchi, Noriyuki, Kim, Bong Gyu, Kim, Jaeheon, Kim, Hyo Ryoung, Kim, Hyun-Goo, Kobayashi, Hideyuki, Kono, Yusuke, Kurayama, Tomoharu, Lee, Changhoon, Lee, Jeong Ae, Lee, Jeewon, Lee, Jung-Won, Lee, Sang Hyun, Lee, Sang-Sung, Minh, Young Chol, Miyazaki, Atsushi, Oh, Se-Jin, Oyama, Tomoaki, Park, Sun-youp, Roh, Duk-Gyoo, Sasao, Tetsuo, Sawada-Satoh, Satoko, Shibata, Katsunori M., Sohn, Bong Won, Song, Min-Gyu, Tamura, Yoshiaki, Wajima, Kiyoaki, Wi, Seog-Oh, Yeom, Jae-Hwan, Yun, Young Joo
Publikováno v:
Matsumoto, N., Hirota, T., & Sugiyama, K. et al. 2014, ApJL, 789, L1
We have carried out the first very long baseline interferometry (VLBI) imaging of 44 GHz class I methanol maser (7_{0}-6_{1}A^{+}) associated with a millimeter core MM2 in a massive star-forming region IRAS 18151-1208 with KaVA (KVN and VERA Array),
Externí odkaz:
http://arxiv.org/abs/1406.2086
Autor:
KAN Ya-Chen, 甘雅珍
86
Tetramethylpyrazine (TMP) is one of the active ingredient of a Chinese herbal medicine. In this study, TMP was tested for its antiplatelet activities in human platelet suspensions. In human platelets, TMP (0.5-1.5 mM) dose-dependently inhibit
Tetramethylpyrazine (TMP) is one of the active ingredient of a Chinese herbal medicine. In this study, TMP was tested for its antiplatelet activities in human platelet suspensions. In human platelets, TMP (0.5-1.5 mM) dose-dependently inhibit
Externí odkaz:
http://ndltd.ncl.edu.tw/handle/43024608195856267977
Autor:
Honma, Mareki, Hirota, Tomoya, Kan-ya, Yukitoshi, Kawaguchi, Noriyuki, Kobayashi, Hideyuki, Kurayama, Tomoharu, Sato, Katsuhisa
We present the results of astrometric observations with VERA toward the H2O maser sources in IRAS 05137+3919, which is thought to be located in the far outer Galaxy. We have derived the parallax of \pi = 0.086 +/- 0.027 mas, which corresponds to the
Externí odkaz:
http://arxiv.org/abs/1101.1354
Autor:
Niinuma, Kotaro, Nagayama, Takumi, Hirota, Tomoya, Honma, Mareki, Motogi, Kazuhito, Nakagawa, Akiharu, Kurayama, Tomoharu, Kan-ya, Yukitoshi, Kawaguchi, Noriyuki, Kobayashi, Hideyuki, Ueno, Yuji
We measured the trigonometric annual parallax of H$_2$O maser source associated with the massive star-forming regions IRAS 06061+2151 with VERA. The annual parallax of $0.496\pm0.031$ mas corresponding to a distance of $2.02^{+0.13}_{-0.12}$ kpc was
Externí odkaz:
http://arxiv.org/abs/1009.5890
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Nakagawa, Akiharu, Tsushima, Miyuki, Ando, Kazuma, Bushimata, Takeshi, Choi, Yoon Kyung, Hirota, Tomoya, Honma, Mareki, Imai, Hiroshi, Iwadate, Kenzaburo, Jike, Takaaki, Kameno, Seiji, Kameya, Osamu, Kamohara, Ryuichi, Kan-Ya, Yukitoshi, Kawaguchi, Noriyuki, Kijima, Masachika, Kim, Mi Kyoung, Kobayashi, Hideyuki, Kuji, Seisuke, Kurayama, Tomoharu, Maeda, Toshihisa, Manabe, Seiji, Maruyama, Kenta, Matsui, Makoto, Matsumoto, Naoko, Miyaji, Takeshi, Nagayama, Takumi, Nakamura, Kayoko, Nyu, Daisuke, Oh, Chung Sik, Omodaka, Toshihiro, Oyama, Tomoaki, Pradel, Nicolas, Sakai, Satoshi, Sasao, Tetsuo, Sato, Katsuhisa, Sato, Mayumi, Shibata, Katsunori M., Suda, Hiroshi, Tamura, Yoshiaki, Ueda, Kousuke, Ueno, Yuji, Yamashita, Kazuyoshi
We present a distance measurement for the semiregular variable S Crateris (S Crt) based on its annual parallax. With the unique dual beam system of the VLBI Exploration for Radio Astrometry (VERA) telescopes, we measured the absolute proper motion of
Externí odkaz:
http://arxiv.org/abs/0808.1151
Autor:
Hirota, Tomoya, Ando, Kazuma, Bushimata, Takeshi, Choi, Yoon Kyung, Honma, Mareki, Imai, Hiroshi, Iwadate, Kenzaburo, Jike, Takaaki, Kameno, Seiji, Kameya, Osamu, Kamohara, Ryuichi, Kan-ya, Yukitoshi, Kawaguchi, Noriyuki, Kijima, Masachika, Kim, Mi Kyoung, Kobayashi, Hideyuki, Kuji, Seisuke, Kurayama, Tomoharu, Manabe, Seiji, Matsui, Makoto, Matsumoto, Naoko, Miyaji, Takeshi, Miyazaki, Atsushi, Nagayama, Takumi, Nakagawa, Akiharu, Namikawa, Daichi, Nyu, Daisuke, Oh, Chung Sik, Omodaka, Toshihiro, Oyama, Tomoaki, Sakai, Satoshi, Sasao, Tetsuo, Sato, Katsuhisa, Sato, Mayumi, Shibata, Katsunori M., Tamura, Yoshiaki, Ueda, Kosuke, Yamashita, Kazuyoshi
Publikováno v:
PASJ, 60, 961-974, 2008
We present results of multi-epoch VLBI observations with VERA (VLBI Exploration of Radio Astrometry) of the 22 GHz H$_{2}$O masers associated with a young stellar object (YSO) IRAS 22198+6336 in a dark cloud L1204G. Based on the phase-referencing VLB
Externí odkaz:
http://arxiv.org/abs/0808.0546
Autor:
Choi, Yoon Kyung, Hirota, Tomoya, Honma, Mareki, Kobayashi, Hideyuki, Bushimata, Takeshi, Imai, Hiroshi, Iwadate, Kenzaburo, Jike, Takaaki, Kameno, Seiji, Kameya, Osamu, Kamohara, Ryuichi, Kan-ya, Yukitoshi, Kawaguchi, Noriyuki, Kijima, Masachika, Kim, Mi Kyoung, Kuji, Seisuke, Kurayama, Tomoharu, Manabe, Seiji, Maruyama, Kenta, Matsui, Makoto, Matsumoto, Naoko, Miyaji, Takeshi, Nagayama, Takumi, Nakagawa, Akiharu, Nakamura, Kayoko, Oh, Chung Sik, Omodaka, Toshihiro, Oyama, Tomoaki, Sakai, Satoshi, Sasao, Tetsuo, Sato, Katsuhisa, Sato, Mayumi, Shibata, Katsunori M., Tamura, Yoshiaki, Thushima, Miyuki, Yamashita, Kazuyoshi
We report astrometric observations of H2O masers around the red supergiant VY Canis Majoris (VY CMa) carried out with VLBI Exploration of Radio Astrometry (VERA). Based on astrometric monitoring for 13 months, we successfully measured a trigonometric
Externí odkaz:
http://arxiv.org/abs/0808.0641
Autor:
Sato, Mayumi, Hirota, Tomoya, Honma, Mareki, Kobayashi, Hideyuki, Sasao, Tetsuo, Bushimata, Takeshi, Choi, Yoon Kyung, Imai, Hiroshi, Iwadate, Kenzaburo, Jike, Takaaki, Kameno, Seiji, Kameya, Osamu, Kamohara, Ryuichi, Kan-ya, Yukitoshi, Kawaguchi, Noriyuki, Kim, Mi Kyoung, Kuji, Seisuke, Kurayama, Tomoharu, Manabe, Seiji, Matsui, Makoto, Matsumoto, Naoko, Miyaji, Takeshi, Nagayama, Takumi, Nakagawa, Akiharu, Nakamura, Kayoko, Oh, Chung Sik, Omodaka, Toshihiro, Oyama, Tomoaki, Sakai, Satoshi, Sato, Katsuhisa, Shibata, Katsunori M., Tamura, Yoshiaki, Yamashita, Kazuyoshi
We have used the Japanese VLBI array VERA to perform high-precision astrometry of an H2O maser source in the Galactic star-forming region NGC 281 West, which has been considered to be part of a 300-pc superbubble. We successfully detected a trigonome
Externí odkaz:
http://arxiv.org/abs/0806.4635