Zobrazeno 1 - 2
of 2
pro vyhledávání: '"Jung, Tae Hyun"'
Autor:
Cui, Yuzhu, Hada, Kazuhiro, Kino, Motoki, Sohn, Bong Won, Park, Jongho, Ro, Hyun Wook, Sawada-Satoh, Satoko, Jiang, Wu, Cui, Lang, Honma, Mareki, Shen, Zhi Qiang, Tazaki, Fumie, An, Tao, Cho, Ilje, Zhao, Guang Yao, Cheng, Xiao Peng, Niinuma, Kotaro, Wajima, Kiyoaki, Zhang, Ying Kang, Kawaguchi, Noriyuki, Algaba, Juan Carlos, Koyama, Shoko, Hirota, Tomoya, Yonekura, Yoshinori, Sakai, Nobuyuki, Xia, Bo, Jiang, Yong Bin, Yu, Lin Feng, Gou, Wei, Hwang, Ju Yeon, Jiang, Yong Chen, Sun, Yun Xia, Jung, Dong Kyu, Kim, Hyo Ryoung, Kim, Jeong Sook, Kobayashi, Hideyuki, Lee, Jee Won, Lee, Jeong Ae, Zhang, Hua, Li, Guang Hui, Xu, Zhi Qiang, Li, Peng, Oh, Jung Hwan, Oh, Se Jin, Oh, Chung Sik, Oyama, Tomoaki, Roh, Duk Gyoo, Shibata, Katsunori M., Guo, Wen, Zhao, Rong Bing, Zhong, Wei Ye, Wang, Jin Qing, Yang, Wen Jun, Yan, Hao, Yeom, Jae Hwan, Li, Bin, Li, Xiao Fei, Yuan, Jian Ping, Dong, Jian, Chen, Zhong, Akiyama, Kazunori, Asada, Keiichi, Byun, Do Young, Hagiwara, Yoshiaki, Hodgson, Jeffrey, Jung, Tae Hyun, Kim, Kee Tae, Lee, Sang Sung, Yi, Kunwoo, Liu, Qing Hui, Liu, Xiang, Lu, Ru Sen, Nakamura, Masanori, Trippe, Sascha, Wang, Na, Wang, Xue Zheng, Zhang, Bo
The East Asian very-long-baseline interferometry (VLBI) Network (EAVN) is a rapidly evolving international VLBI array that is currently promoted under joint efforts among China, Japan, and Korea. EAVN aims at forming a joint VLBI Network by combining
Externí odkaz:
http://arxiv.org/abs/2104.05525
Autor:
Dodson, Richard, Rioja, María J., Jung, Tae-Hyun, Sohn, Bong-Won, Byun, Do-Young, Cho, Se-Hyung, Lee, Sang-Sung, Kim, Jongsoo, Kim, Kee-Tae, Oh, Chung-Sik, Han, Seog-Tae, Je, Do-Heung, Chung, Moon-Hee, Wi, Seog-Oh, Kang, Jiman, Lee, Jung-Won, Chung, Hyunsoo, Kim, Hyo-Ryoung, Kim, Hyun-Goo, Lee, Chang-Hoon, Roh, Duk-Gyoo, Oh, Se-Jin, Yeom, Jae-Hwan, Song, Min-Gyu, Kang, Yong-Woo
Oxygen-rich Asymptotic Giant Branch (AGB) stars can be intense emitters of SiO ($v$=1 and 2, J=1$\rightarrow$0) and H$_2$O maser lines at 43 and 22 GHz, respectively. VLBI observations of the maser emission provide a unique tool to probe the innermos
Externí odkaz:
http://arxiv.org/abs/1408.3513