Zobrazeno 1 - 10
of 87
pro vyhledávání: '"L. Viktor Tóth"'
Autor:
Anindya Saha, Anandmayee Tej, Hong-Li Liu, Tie Liu, Guido Garay, Paul F. Goldsmith, Chang Won Lee, Jinhua He, Mika Juvela, Leonardo Bronfman, Tapas Baug, Enrique Vázquez-Semadeni, Patricio Sanhueza, Shanghuo Li, James O. Chibueze, N. K. Bhadari, Lokesh K. Dewangan, Swagat Ranjan Das, Feng-Wei Xu, Namitha Issac, Jihye Hwang, L. Viktor Tóth
Publikováno v:
The Astrophysical Journal Letters, Vol 970, Iss 2, p L40 (2024)
Using new continuum and molecular line data from the Atacama Large Millimeter/submillimeter Array Three-millimeter Observations of Massive Star-forming Regions (ATOMS) survey and archival Very Large Array, 4.86 GHz data, we present direct observation
Externí odkaz:
https://doaj.org/article/4281b39612e345258e6c09d6a52d6cfb
Autor:
Fengwei Xu, Ke Wang, Tie Liu, David Eden, Xunchuan Liu, Mika Juvela, Jinhua He, Doug Johnstone, Paul Goldsmith, Guido Garay, Yuefang Wu, Archana Soam, Alessio Traficante, Isabelle Ristorcelli, Edith Falgarone, Huei-Ru Vivien Chen, Naomi Hirano, Yasuo Doi, Woojin Kwon, Glenn J. White, Anthony Whitworth, Patricio Sanhueza, Mark G. Rawlings, Dana Alina, Zhiyuan Ren, Chang Won Lee, Ken’ichi Tatematsu, Chuan-Peng Zhang, Jianjun Zhou, Shih-Ping Lai, Derek Ward-Thompson, Sheng-Yuan Liu, Qilao Gu, Eswaraiah Chakali, Lei Zhu, Diego Mardones, L. Viktor Tóth
Publikováno v:
The Astrophysical Journal Letters, Vol 963, Iss 1, p L9 (2024)
High-latitude (∣ b ∣ > 30°) molecular clouds have virial parameters that exceed 1, but whether these clouds can form stars has not been studied systematically. Using JCMT SCUBA-2 archival data, we surveyed 70 fields that target high-latitude Pla
Externí odkaz:
https://doaj.org/article/8e3aa8d23bb6459c80060fd043424f16
Autor:
Xiaofeng Mai, Tie Liu, Xunchuan Liu, Lei Zhu, Guido Garay, Paul F. Goldsmith, Mika Juvela, Hongli Liu, Emma Mannfors, Anandmayee Tej, Patricio Sanhueza, Shanghuo Li, Fengwei Xu, Enrique Vazquez Semadeni, Wenyu Jiao, Yaping Peng, T. Baug, Aiyuan Yang, Lokesh Dewangan, Leonardo Bronfman, Gilberto C. Gómez, Aina Palau, Chang Won Lee, Sheng-Li Qin, Ken’ichi Tatematsu, James O. Chibueze, Dongting Yang, Xing Lu, Qiuyi Luo, Qilao Gu, Namitha Issac, Suinan Zhang, Pak-Shing Li, Bo Zhang, L. Viktor Tóth
Publikováno v:
The Astrophysical Journal Letters, Vol 961, Iss 2, p L35 (2024)
Only a handful of massive starless core candidates have been discovered so far, but none of them have been fully confirmed. Within the MM1 clump in the filamentary infrared dark cloud G34.43+0.24 that was covered by the Atacama Large Millimeter/submi
Externí odkaz:
https://doaj.org/article/a6dc87487ce242908bb19ed1ca15b39f
Publikováno v:
Universe, Vol 8, Iss 7, p 342 (2022)
Gamma-ray bursts (GRBs) are the most luminous objects known: they outshine their host galaxies, making them ideal candidates for probing large-scale structure. Our aim is to determine the Spatial Two-Point Correlation Function of the GRBs with spectr
Externí odkaz:
https://doaj.org/article/ea94ceb3cd854f629b660bfc8d363ba9
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 4 (2017)
Active galactic nuclei (AGN) are prominent astrophysical objects that can be observed throughout the whole Universe. To understand the underlying physical processes and the different appearance of AGN types, extensive samples are needed. Nowadays, va
Externí odkaz:
https://doaj.org/article/1f8c0e00253d4b08a45c064a7a211a92
Autor:
Ken'ichi Tatematsu, Eswaraiah Chakali, Feng-Wei Xu, Mika Juvela, E. Mannfors, Qiu-Yi Luo, Qizhou Zhang, S. N. Zhang, Sheng-Li Qin, Lokesh K. Dewangan, Ke Wang, L. Viktor Tóth, Junzhi Wang, Tie Liu, Rong Liu, Zhiyuan Ren, Leonardo Bronfman, Paul F. Goldsmith, T. Baug, Jin-Zeng Li, Shanghuo Li, Pak Shing Li, Jianwen Zhou, X.-W. Liu, Xi Chen, Chang Won Lee, Somnath Dutta, Hong-Li Liu, Yong Zhang, Di Li, Anandmayee Tej, Chao Zhang, Archana Soam, Yuefang Wu, Anindya Saha, Amelia M. Stutz, Namitha Issac, Mengyao Tang
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 510:5009-5022
We present new 3-mm continuum and molecular lines observations from the ATOMS survey towards the massive protostellar clump, MM1, located in the filamentary infrared dark cloud (IRDC), G034.43+00.24 (G34). The lines observed are the tracers of either
Autor:
Rong Liu, Tie Liu, Gang Chen, Hong-Li Liu, Ke Wang, Jin-Zeng Li, Chang Won Lee, Xunchuan Liu, Mika Juvela, Guido Garay, Lokesh Dewangan, Archana Soam, Leonardo Bronfman, Jinhua He, Chakali Eswaraiah, Si-Ju Zhang, Yong Zhang, Feng-Wei Xu, L Viktor Tóth, Zhi-Qiang Shen, Shanghuo Li, Yue-Fang Wu, Sheng-Li Qin, Zhiyuan Ren, Guoyin Zhang, Anandmayee Tej, Paul F Goldsmith, Tapas Baug, Qiuyi Luo, Jianwen Zhou, Chang Zhang
To understand the nature of SiO emission, we conducted ACA observations of the SiO (2-1) lines toward 146 massive star-forming regions, as part of the ALMA Three-millimeter Observations of Massive Star-forming regions (ATOMS) survey. We detected SiO
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e93c6e2c1cd0f4c267275feec715bbe7
http://hdl.handle.net/10138/352548
http://hdl.handle.net/10138/352548
Autor:
Nofoz Suleiman, Akatoki Noboriguchi, Yoshiki Toba, Lajos G Balázs, Denis Burgarella, Timea Kovács, Gábor Marton, Mohammed Talafha, Sándor Frey, L Viktor Tóth
Publikováno v:
Publications of the Astronomical Society of Japan
Publications of the Astronomical Society of Japan, 2022, ⟨10.1093/pasj/psac061⟩
Publications of the Astronomical Society of Japan, 2022, ⟨10.1093/pasj/psac061⟩
The aim of this study is to characterize the physical and statistical properties of a sample of infrared-bright dust-obscured galaxies (DOGs) by fitting their spectral energy distributions (SEDs). We examined 28 DOGs at redshifts 0.47 ≤ z ≤ 1.63
Autor:
Juan Li, Ya-Ping Peng, Yong Zhang, Diego Mardones, Sung-ju Kang, X.-W. Liu, Yuefang Wu, Jeong-Eun Lee, Sheng-Yuan Liu, Chang Won Lee, Amelia M. Stutz, Hong-Li Liu, Mengyao Tang, Maria Cunningham, Eswaraiah Chakali, Rodrigo H. Álvarez-Gutiérrez, Mika Juvela, Hee-Weon Yi, Qizhou Zhang, Chao Zhang, Zhi-Qiang Shen, Qiu-Yi Luo, Feng-Wei Xu, Leonardo Bronfman, Guido Garay, Zhiyuan Ren, Shanghuo Li, Neal J. Evans, Rong Liu, Sheng-Li Qin, Jianwen Zhou, Yu Wang, Kee-Tae Kim, Namitha Issac, Tomoya Hirota, Feng-Yao Zhu, Anandmayee Tej, Pak Shing Li, Junzhi Wang, Jingwen Wu, Lokesh K. Dewangan, Ke Wang, L. Viktor Tóth, Tie Liu, Archana Soam, Ken'ichi Tatematsu, Di Li, Qiaowei Xue, Jin-Zeng Li, Paul F. Goldsmith, Hyeong-Sik Yun, T. Baug, Isabelle Ristorcelli
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2021, 505, pp.2801-2818. ⟨10.1093/mnras/stab1352⟩
Monthly Notices of the Royal Astronomical Society, 2021, 505, pp.2801-2818. ⟨10.1093/mnras/stab1352⟩
We have identified 453 compact dense cores in 3 mm continuum emission maps in the ATOMS (ALMA Three-millimeter Observations of Massive Star-forming regions) survey, and compiled three catalogues of high-mass star forming cores. One catalogue, referre
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::abd2621fed5b0e3438c4d6e09bab7e1e
http://hdl.handle.net/10138/341135
http://hdl.handle.net/10138/341135
Autor:
Hong-Li Liu, Shanghuo Li, Ke Wang, Qizhou Zhang, Paul F. Goldsmith, Mengyao Tang, Ken'ichi Tatematsu, T. Baug, Anandmayee Tej, Tomoya Hirota, Di Li, Yuefang Wu, Chang Won Lee, Leonardo Bronfman, Kee-Tae Kim, L. Viktor Tóth, Tie Liu
With the aim of understanding the role of outflows in star formation, we performed a statistical study of the physical parameters of outflows in eleven massive protoclusters associated with ultra-compact HII regions. A total of 106 outflow lobes are
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7bc0c612a6ab01e8a4c3a57f407502a9