Zobrazeno 1 - 10
of 2 998
pro vyhledávání: '"Sanhueza P"'
Autor:
Liu, Chun-Fan, Shang, Hsien, Johnstone, Doug, Ai, Tsung-Han, Lee, Tsz Ming, Krasnopolsky, Ruben, Hirano, Naomi, Dutta, Somnath, Hsu, Shih-Ying, López-Vázquez, Jesús Alejandro, Liu, Sheng-Yuan, Liu, Tie, Tatematsu, Ken'ichi, Zhang, Qizhou, Rawlings, Mark G., Eden, David, Ren, Zhiyuan, Sanhueza, Patricio, Kwon, Woojin, Lee, Chang Won, Kuan, Yi-Jehng, Bandopadhyay, Somdeb, Väisälä, Miikka S., Lee, Chin-Fei, Das, Indrani
The Atacama Large Millimeter/submillimeter Array Survey of Orion Planck Galactic Cold Clumps (ALMASOP) reveals complex nested morphological and kinematic features of molecular outflows through the CO (J = 2 - 1) and SiO (J = 5 - 4) emission. We chara
Externí odkaz:
http://arxiv.org/abs/2411.08827
Autor:
Zhang, Siju, Liu, Tie, Wang, Ke, Zavagno, Annie, Garay, Guido, Liu, Hongli, Xu, Fengwei, Liu, Xunchuan, Sanhueza, Patricio, Soam, Archana, Zhou, Jian-wen, Li, Shanghuo, Goldsmith, Paul F., Zhang, Yong, Chibueze, James O., Lee, Chang Won, Hwang, Jihye, Bronfman, Leonardo, Dewangan, Lokesh K.
Fragmentation and evolution for the molecular shells of the compact HII regions are less explored compared to their evolved counterparts. We map nine compact HII regions with a typical diameter of 0.4 pc that are surrounded by molecular shells traced
Externí odkaz:
http://arxiv.org/abs/2410.17455
Autor:
Gu, Qi-Lao, Liu, Tie, Shen, Zhi-Qiang, Jiao, Sihan, Montillaud, Julien, Juvela, Mika, Lu, Xing, Lee, Chang Won, Liu, Junhao, Li, Pak Shing, Liu, Xunchuan, Johnstone, Doug, Kwon, Woojin, Kim, Kee-Tae, Tatematsu, Ken'ichi, Sanhueza, Patricio, Ristorcelli, Isabelle, Koch, Patrick, Zhang, Qizhou, Pattle, Kate, Hirano, Naomi, Alina, Dana, Di Francesco, James
We present 850 {\mu}m thermal dust polarization observations with a resolution of 14.4"(~ 0.13 pc) towards an infrared dark cloud G16.96+0.27 using JCMT/POL-2. The average magnetic field orientation, which roughly agrees with the larger-scale magneti
Externí odkaz:
http://arxiv.org/abs/2410.15913
Autor:
Yang, Dongting, Liu, HongLi, Liu, Tie, Tej, Anandmayee, Liu, Xunchuan, He, Jinhua, Garay, Guido, Stutz, Amelia, Zhu, Lei, Qin, Sheng-Li, Xu, Fengwei, Li, Pak-Shing, Juvela, Mika, Garcia, Pablo, Goldsmith, Paul F., Zhang, Siju, Tang, Xindi, Sanhueza, Patricio, Li, Shanghuo, Lee, Chang Won, Das, Swagat Ranjan, Jiao, Wenyu, Mai, Xiaofeng, Gorai, Prasanta, Zhang, Yichen, Ren, Zhiyuan, Toth, L. Viktor, Hwang, Jihye, Bronfman, Leonardo, Tatematsu, Kenichi, Dewangan, Lokesh, Chibueze, James O., Zhang, Suinan, Wu, Gang, Xie, Jinjin
In this paper, we present a detailed analysis of the IRS 17 filament within the intermediate-mass protocluster IRAS 08448-4343 (of $\sim\,10^3\,\rm L_{\odot}$), using ALMA data from the ATOMS 3-mm and QUARKS 1.3-mm surveys. The IRS 17 filament, which
Externí odkaz:
http://arxiv.org/abs/2410.15333
Autor:
Sandoval-Garrido, N. A., Stutz, A. M., Álvarez-Gutiérrez, R. H., Galván-Madrid, R., Motte, F., Ginsburg, A., Cunningham, N., Reyes-Reyes, S., Redaelli, E., Bonfand, M., Salinas, J., Koley, A., Braine, J., Bronfman, L., Busquet, G., Csengeri, T., Di Francesco, J., Fernández-López, M., Garcia, P., Gusdorf, A., Liu, H. -L., Sanhueza, P.
ALMA-IMF observed 15 massive protoclusters capturing multiple spectral lines and the continuum emission. We focus on the G351.77 protocluster ($\sim$ 2500 M$_{\odot}$, estimated from single-dish continuum observations) located at 2 kpc. We trace the
Externí odkaz:
http://arxiv.org/abs/2410.09843
Autor:
Das, Swagat R., Merello, Manuel, Bronfman, Leonardo, Liu, Tie, Garay, Guido, Stutz, Amelia, Mardones, Diego, Zhou, Jian-Wen, Sanhueza, Patricio, Liu, Hong-Li, Vázquez-Semadeni, Enrique, Gómez, Gilberto C., Palau, Aina, Tej, Anandmayee, Xu, Feng-Wei, Baug, Tapas, Dewangan, Lokesh K., He, Jinhua, Zhu, Lei, Li1, Shanghuo, Juvela, Mika, Saha, Anindya, Issac, Namitha, Hwang, Jihye, Nazeer, Hafiz, Toth, L. Viktor
Hub-filament systems are considered as natural sites for high-mass star formation. Kinematic analysis of the surroundings of hub-filaments is essential to better understand high-mass star formation within such systems. In this work, we present a deta
Externí odkaz:
http://arxiv.org/abs/2409.19204
Autor:
Hsu, Shih-Ying, Lee, Chin-Fei, Liu, Sheng-Yuan, Johnstone, Doug, Liu, Tie, Takahashi, Satoko, 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, Chang Won, Lee, Jeong-Eun, Li, Shanghuo, Liu, Chun-Fan, Liu, Xunchuan, Luo, Qiuyi, Qin, Sheng-Li, Sahu, Dipen, Sanhueza, Patricio, Shang, Hsien, Tatematsu, Kenichi, Yang, Yao-Lun
HOPS 87 is a Class 0 protostellar core known to harbor an extremely young bipolar outflow and a hot corino. We report the discovery of localized, chemically rich regions near the bases of the two-lobe bipolar molecular outflow in HOPS 87 containing m
Externí odkaz:
http://arxiv.org/abs/2409.14445
Autor:
Shen, Xianjin, Liu, Hong-Li, Ren, Zhiyuan, Tej, Anandmayee, Li, Di, Liu, Hauyu Baobab, Fuller, Gary A., Xie, Jinjin, Jiao, Sihan, Yang, Aiyuan, Koch, Patrick M., Xu, Fengwei, Sanhueza, Patricio, Diep, Pham N., Peretto, Nicolas, Yadav, Ram K., Kramer, Busaba H., Sugiyama, Koichiro, Rawlings, Mark, Lee, Chang Won, Tatematsu, Ken'ichi, Harsono, Daniel, Eden, David, Kwon, Woojin, Tsai, Chao-Wei, White, Glenn, Kim, Kee-Tae, Liu, Tie, Wang, Ke, Zhang, Siju, Jiao, Wenyu, Yang, Dongting, Swagat, Das R., Wu, Jingwen, Wang, Chen
Filaments are believed to play a key role in high-mass star formation. We present a systematic study of the filaments and their hosting clumps in the G35 molecular complex using JCMT SCUBA-2 850 $\micron$ continuum data. We identified five clouds in
Externí odkaz:
http://arxiv.org/abs/2409.05492
Autor:
Hàn, Hiêp, Lang, Richard, Marciano, João Pedro, Pavez-Signé, Matías, Sanhueza-Matamala, Nicolás, Treglown, Andrew, Zárate-Guerén, Camila
We study conditions under which an edge-coloured hypergraph has a particular substructure that contains more than the trivially guaranteed number of monochromatic edges. Our main result solves this problem for perfect matchings under minimum degree c
Externí odkaz:
http://arxiv.org/abs/2408.11016
Autor:
Zapata, Luis A., Fernández-López, Manuel, Sanhueza, Patricio, Girart, Josep M., Rodríguez, Luis F., Cortes, Paulo, Patrick, Koch, Beltrán, María T., Pattle, Kate, Beuther, Henrik, Saha, Piyali, Jiao, Wenyu, Xu, Fengwei, Lu, Xing Walker, Olguin, Fernando, Li, Shanghuo, Stephens, Ian W., Kang, Ji-hyun, Cheng, Yu, Choudhury, Spandan, Morii, Kaho, Chung, Eun Jung, Wang, Jia-Wei, Hwang, Jihye, Lyo, A-Ran, Zhang, Qizhou, Chen, Huei-Ru Vivien
The formation of the massive stars, and in particular, the role that the magnetic fields play in their early evolutionary phase is still far from being completely understood. Here, we present Atacama Large Millimeter/Submillimeter Array (ALMA) 1.2 mm
Externí odkaz:
http://arxiv.org/abs/2408.10199