H
Hua-bai Li
Researcher at The Chinese University of Hong Kong
Publications - 89
Citations - 2994
Hua-bai Li is an academic researcher from The Chinese University of Hong Kong. The author has contributed to research in topics: Magnetic field & Molecular cloud. The author has an hindex of 31, co-authored 81 publications receiving 2608 citations. Previous affiliations of Hua-bai Li include Max Planck Society & Harvard University.
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Magnetic Fields and Massive Star Formation
Qizhou Zhang,Keping Qiu,Josep M. Girart,Hauyu,Liu,Ya-Wen Tang,Patrick M. Koch,Zhi-Yun Li,Eric Keto,Paul T. P. Ho,Ramprasad Rao,Shih-Ping Lai,Tao-Chung Ching,P. Frau,How-Huan Chen,Hua-bai Li,Marco Padovani,Sylvain Bontemps,Timea Csengeri,Carmen Juárez +19 more
TL;DR: In this article, the role of magnetic fields in the formation of dense cores was investigated through dust polarization at 870$m obtained with the Submillimeter Array (SMA).
Journal ArticleDOI
Magnetic fields and massive star formation
Qizhou Zhang,Keping Qiu,Josep M. Girart,Hauyu Baobab Liu,Ya-Wen Tang,Patrick M. Koch,Zhi-Yun Li,Eric Keto,Paul T. P. Ho,Paul T. P. Ho,Ramprasad Rao,Shih-Ping Lai,Shih-Ping Lai,Tao-Chung Ching,Tao-Chung Ching,P. Frau,How-Huan Chen,Hua-bai Li,Marco Padovani,Sylvain Bontemps,Timea Csengeri,Carmen Juárez +21 more
TL;DR: In this paper, the role of magnetic fields in the formation of dense cores was investigated through dust polarization at 870 μm obtained with the Submillimeter Array (SMA).
Journal ArticleDOI
The link between magnetic fields and filamentary clouds: bimodal cloud orientations in the Gould Belt
TL;DR: In this paper, the orientations of filamentary molecular clouds in the Gould Belt and their local intercloud media (ICM) magnetic fields are studied using near-infrared dust extinction maps and optical stellar polarimetry data.
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Self-similar fragmentation regulated by magnetic fields in a region forming massive stars.
Hua-bai Li,Ka Ho Yuen,Frank Otto,Po Kin Leung,T. K. Sridharan,Qizhou Zhang,Hauyu Liu,Ya-Wen Tang,Keping Qiu +8 more
TL;DR: It is concluded that magnetic fields have a crucial role in the fragmentation of NGC 6334, a region forming massive stars, on the 100 to 0.01 parsec scale.
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Anchoring magnetic field in turbulent molecular clouds
Hua-bai Li,C. Darren Dowell,C. Darren Dowell,Alyssa A. Goodman,Roger H. Hildebrand,Giles Novak +5 more
TL;DR: In this paper, the role of magnetic fields in star formation was investigated and a significant correlation was found for field directions detected from the two extremes, however, only the sub-Alfvenic cases result in field orientations consistent with their observations.