activity
20092023
most citedHierarchical fragmentation and differential star formation in the Galactic "Snake": infrared dark cloud G11.11-0.12

264 citations · 3.5k across the 86 of their papers we have counts for

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Showing astro-ph.SRShow all

9 papers · 1 filter

astro-ph.SR2020★ 34 cited

Fragmentation of star-forming filaments in the X-shape Nebula of the California molecular cloud

Guo Yin Zhang, Ph. Andre, A. Menshchikov +1

Dense molecular filaments are central to the star formation process, but the detailed manner in which they fragment into prestellar cores is not yet well understood. Here, we inves…

astro-ph.SR2019★ 4 cited

Sequential Star Formation in the filamentary structures of Planck Galactic cold clump G181.84+0.31

Lixia Yuan, Ming Zhu, Tie Liu +7

We present a multi-wavelength study of the Planck cold clump G181.84+0.31, which is located at the northern end of the extended filamentary structure S242. We have extracted 9 comp…

astro-ph.SR2018★ 11 cited

Compressed magnetic field in the magnetically-regulated global collapsing clump of G9.62+0.19

Tie Liu, Kee-Tae Kim, Sheng-Yuan Liu +22

How stellar feedback from high-mass stars (e.g., H{\sc ii} regions) influences the surrounding interstellar medium and regulates new star formation is still unclear. To address thi…

astro-ph.SR2015★ 191 cited

Fragmentation of Molecular Clumps and Formation of Protocluster

Qizhou Zhang, Ke Wang, Xing Lu +1

Sufficiently massive clumps of molecular gas collapse under self-gravity and fragment to spawn a cluster of stars that have a range of masses. We investigate observationally the ea…

astro-ph.SR2015★ 9 cited

Extremely Energetic Outflow and Decelerated Expansion in W49N

Tie Liu, Kee-Tae Kim, Yuefang Wu +10

W49N is a mini-starburst in the Milky Way and thus an ideal laboratory for high-mass star formation studies. Due to its large distance (11.1 kpc), the kinematics in…

astro-ph.SR2014

Follow-up observations toward Planck cold clumps with ground-based radio telescopes

Tie Liu, Yuefang Wu, Diego Mardones +26

The physical and chemical properties of prestellar cores, especially massive ones, are still far from being well understood due to the lack of a large sample. The low dust temperat…