Zobrazeno 1 - 10
of 86
pro vyhledávání: '"Hsu, Shih-Ying"'
Autor:
Hirano, Naomi, Sahu, Dipen, Liu, Sheng-Yaun, Liu, Tie, Tatematsu, Ken'ichi, Dutta, Somnath, Li, Shanghuo, Lee, Chin-Fei, Li, Pak Shing, Hsu, Shih-Ying, Lin, Sheng-Jun, Johnstone, Doug, Bronfman, Leonardo, Chen, Huei-Ru Vivien, Eden, David J., Kuan, Yi-Jehng, Kwon, Woojin, Lee, Chang Won, Liu, Hong-Li, Rawlings, Mark G., Ristorcelli, Isabelle, Traficante, Alessio
The internal structure of the prestellar core G208.68-19.02-N2 (G208-N2) in the Orion Molecular Cloud 3 (OMC-3) region has been studied with the Atacama Large Millimeter/submillimeter Array (ALMA). The dust continuum emission revealed a filamentary s
Externí odkaz:
http://arxiv.org/abs/2311.05308
Autor:
Hsu, Shih-Ying, Liu, Sheng-Yuan, Johnstone, Doug, Liu, Tie, Bronfman, Leonardo, Chen, Huei-Ru Vivien, Dutta, Somnath, Eden, David J., Evans II, Neal J., Hirano, Naomi, Juvela, Mika, Kuan, Yi-Jehng, Kwon, Woojin, Lee, Chin-Fei, Lee, Chang Won, Lee, Jeong-Eun, Li, Shanghuo, Liu, Chun-Fan, Liu, Xunchuan, Luo, Qiuyi, Qin, Sheng-Li, Rawlings, Mark G., Sahu, Dipen, Sanhueza, Patricio, Shang, Hsien, Tatematsu, Kenichi, Yang, Yao-Lun
Hot corinos are of great interest due to their richness in interstellar complex organic molecules (COMs) and the consequent potential prebiotic connection to solar-like planetary systems. Recent surveys have reported an increasing number of hot corin
Externí odkaz:
http://arxiv.org/abs/2308.05494
Autor:
Dutta, Somnath, Lee, Chin-Fei, Johnstone, Doug, Lee, Jeong-Eun, Hirano, Naomi, Di Francesco, James, Moraghan, Anthony, Liu, Tie, Sahu, Dipen, Liu, Sheng-Yuan, Tatematsu, Kenichi, Lee, Chang Won, Li, Shanghuo, Eden, David, Juvela, Mika, Bronfman, Leonardo, Hsu, Shih-Ying, Kim, Kee-Tae, Kwon, Woojin, Sanhueza, Patricio, Lopez-Vazquez, Jesus Alejandro, Luo, Qiuyi, Yi, Hee-Weon
Protostellar outflows and jets are almost ubiquitous characteristics during the mass accretion phase, and encode the history of stellar accretion, complex-organic molecule (COM) formation, and planet formation. Episodic jets are likely connected to e
Externí odkaz:
http://arxiv.org/abs/2306.15346
Autor:
Luo, Qiu-yi, Liu, Tie, Lee, Aaron T., Offner, Stella S. R., di Francesco, James, Johnstone, Doug, Juvela, Mika, Goldsmith, Paul F., Qin, Sheng-Li, Mai, Xiaofeng, Liu, Xun-chuan, Sanhueza, Patricio, Xu, Feng-Wei, Tatematsu, Ken'ichi, Dutta, Somnath, Chen, Huei-Ru Vivien, Li, Shanghuo, Yang, Aiyuan, Liu, Sheng-Yuan, Lee, Chin-Fei, Hirano, Naomi, Lee, Chang Won, Sahu, Dipen, Shang, Hsien, Hsu, Shih-Ying, Bronfman, Leonardo, Kwon, Woojin, Rawlings, M. G., Eden, David, Lu, Xing, Gu, Qi-lao, Ren, Zhiyuan, Ward-Thompson, D, Shen, Zhi-Qiang
One of the most poorly understood aspects of low-mass star formation is how multiple-star systems are formed. Here we present the results of Atacama Large Millimeter/submillimeter Array (ALMA) Band-6 observations towards a forming quadruple protostel
Externí odkaz:
http://arxiv.org/abs/2306.07839
Autor:
Sahu, Dipen, Liu, Sheng-Yuan, Johnstone, Doug, Liu, Tie, Evans II, Neal J., Hirano, Naomi, Tatematsu, Kenichi, Di Francesco, James, Lee, Chin-Fei, Kim, Kee-Tae, Dutta, Somnath, Hsu, Shih-Ying, Li, Shanghuo, Luo, Qiu-Yi, Sanhueza, Patricio, Shang, Hsien, Traficante, Alessio, Juvela, Mika, Lee, Chang Won, Eden, David J., Goldsmith, Paul F., Bronfman, Leonardo, Kwon, Woojin, Lee, Jeong-Eun, Kuan, Yi-Jehng, Ristorcelli, Isabelle
Starless cores represent the initial stage of evolution toward (proto)star formation, and a subset of them, known as prestellar cores, with high density (~ 10^6 cm^-3 or higher) and being centrally concentrated are expected to be embryos of (proto)st
Externí odkaz:
http://arxiv.org/abs/2302.07634
Autor:
TAROGE Collaboration, Wang, Shih-Hao, Nam, Jiwoo, Chen, Pisin, Chen, Yaocheng, Choi, Taejin, Ham, Young-bae, Hsu, Shih-Ying, Huang, Jian-Jung, Huang, Ming-Huey A., Jee, Geonhwa, Jung, Jongil, Kim, Jieun, Kuo, Chung-Yun, Kwon, Hyuck-Jin, Lee, Changsup, Leung, Chung-Hei, Liu, Tsung-Che, Shiao, Yu-Shao J., Shin, Bok-Kyun, Wang, Min-Zu, Wang, Yu-Hsin, Collaboration, ARIANNA, Anker, Astrid, Barwick, Steven W., Besson, Dave Z., Bouma, Sjoerd, Cataldo, Maddalena, Gaswint, Geoffrey, Glaser, Christian, Hallmann, Steffen, Hanson, Jordan C., Henrichs, Jakob, Kleinfelder, Stuart A., Lahmann, Robert, Meyers, Zachary S., Nelles, Anna, Novikov, Alexander, Paul, Manuel P., Pyras, Lilly, Persichilli, Christopher, Plaisier, Ilse, Rice-Smith, Ryan, Seikh, Mohammad F. H., Tatar, Joulien, Welling, Christoph, Zhao, Leshan
Publikováno v:
JCAP11(2022)022
TAROGE-M is a self-triggered radio antenna array atop the 2700 m high Mt. Melbourne in Antarctica, designed to detect impulsive geomagnetic emission from extensive air showers induced by ultra-high energy (UHE) particles beyond 0.1 EeV, including cos
Externí odkaz:
http://arxiv.org/abs/2207.10616
Autor:
Jhan, Kai-Syun, Lee, Chin-Fei, Johnstone, Doug, Liu, Tie, Liu, Sheng-Yuan, Hirano, Naomi, Tatematsu, Kenichi, Dutta, Somnath, Moraghan, Anthony, Shang, Hsien, Lee, Jeong-Eun, Li, Shanghuo, Liu, Chun-Fan, Hsu, Shih-Ying, Kwon, Woojin, Sahu, Dipen, Liu, Xun-Chuan, Kim, Kee-Tae, Luo, Qiuyi, Qin, Sheng-Li, Sanhueza, Patricio, Bronfman, Leonardo, Qizhou, Zhang, Eden, David, Traficante, Alessio, Lee, Chang Won
We have selected six sources (G209.55-19.68S2, G205.46-14.56S1$_{-}$A, G203.21-11.20W2, G191.90-11.21S, G205.46-14.56S3, and G206.93-16.61W2) from the Atacama Large Millimeter/submillimeter Array Survey of Orion Planck Galactic Cold Clumps (ALMASOP),
Externí odkaz:
http://arxiv.org/abs/2204.12731
Autor:
Dutta, Somnath, Lee, Chin-Fei, Hirano, Naomi, Liu, Tie, Johnstone, Doug, Liu, Sheng-Yuan, Tatematsu, Kenichi, Goldsmith, Paul F., Sahu, Dipen, Evans, Neal J., Sanhueza, Patricio, Kwon, Woojin, Qin, Sheng-Li, Samal, Manash Ranjan, Zhang, Qizhou, Kim, Kee-Tae, Shang, Hsien, Lee, Chang Won, Moraghan, Anthony, Jhan, Kai-Syun, Li, Shanghuo, Lee, Jeong-Eun, Traficante, Alessio, Juvela, Mika, Bronfman, Leonardo, Eden, David, Soam, Archana, He, Jinhua, Liu, Hong-li, Kuan, Yi-Jehng, Pelkonen, Veli-Matti, Luo, Qiuyi, Yi, Hee-Weon, Hsu, Shih-Ying
Protostellar outflows and jets play a vital role in star formation as they carry away excess angular momentum from the inner disk surface, allowing the material to be transferred toward the central protostar. Theoretically, low velocity and poorly co
Externí odkaz:
http://arxiv.org/abs/2204.06661
Autor:
Tatematsu, Ken'ichi, Yeh, You-Ting, Hirano, Naomi, Liu, Sheng-Yuan, Liu, Tie, Dutta, Somnath, Sahu, Dipen, Evans II, Neal J., Juvela, Mika, Yi, Hee-Weon, Lee, Jeong-Eun, Sanhueza, Patricio, Li, Shanghuo, Eden, David, Kim, Gwanjeong, Lee, Chin-Fei, Wu, Yuefang, Kim, Kee-Tae, T'oth, L. Viktor, Choi, Minho, Kang, Miju, Thompson, Mark A., Fuller, Gary A., Di Li, 20, Wang, Ke, Sakai, Takeshi, Kandori, Ryo, Hsu, Shih-Ying, Chiong, Chau-Ching, collaboration, JCMT Large Program SCOPE, collaboration, ALMASOP
Publikováno v:
Astrophysical J. 931 (2022) 33
In this study, 36 cores (30 starless and 6 protostellar) identified in Orion were surveyed to search for inward motions. We used the Nobeyama 45 m radio telescope, and mapped the cores in the $J = 1\rightarrow0$ transitions of HCO$^+$, H$^{13}$CO$^+$
Externí odkaz:
http://arxiv.org/abs/2203.12885
Autor:
Qin, Sheng-Li, Liu, Tie, Liu, Xunchuan, Goldsmith, Paul F., Li, Di, Zhang, Qizhou, Liu, Hong-Li, Wu, Yuefang, Bronfman, Leonardo, Juvela, Mika, Lee, Chang Won, Garay, Guido, Zhang, Yong, He, Jinhua, Hsu, Shih-Ying, Shen, Zhi-Qiang, Lee, Jeong-Eun, Wang, Ke, Tang, Ningyu, Tang, Mengyao, Zhang, Chao, Yue, Yinghua, Xue, Qiaowei, Li, Shang-Huo, Peng, Yaping, Dutta, Somnath, Jixing, Ge, Xu, Fengwei, Chen, Longfei, Baug, Tapas, dewanggan, Lokesh, Tej, Anandmayee
Hot cores characterized by rich lines of complex organic molecules are considered as ideal sites for investigating the physical and chemical environments of massive star formation. We present a search for hot cores by using typical nitrogen- and oxyg
Externí odkaz:
http://arxiv.org/abs/2201.10044