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20072023
most citedProbing the initial conditions of high-mass star formation. II. Fragmentation, stability, and chemistry

163 citations · 1.1k across the 46 of their papers we have counts for

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Showing 2023Show all

5 papers · 1 filter

astro-ph.GA2023★ 6 cited

Mapping gravity in stellar nurseries -- establishing the effectiveness of 2D acceleration maps

Zhen-Zhen He, Guang-Xing Li, Andreas Burkert

Gravity is the driving force of star formation. Although gravity is caused by the presence of matter, its role in complex regions is still unsettled. One effective way to study the…

astro-ph.GA2023★ 14 cited

The JCMT BISTRO Survey: Studying the Complex Magnetic Field of L43

Janik Karoly, Derek Ward-Thompson, Kate Pattle +155

We present observations of polarized dust emission at 850 m from the L43 molecular cloud which sits in the Ophiuchus cloud complex. The data were taken using SCUBA-2/POL-2 on th…

astro-ph.GA2023★ 11 cited

First BISTRO observations of the dark cloud Taurus L1495A-B10: the role of the magnetic field in the earliest stages of low-mass star formation

Derek Ward-Thompson, Janik Karoly, Kate Pattle +155

We present BISTRO Survey 850 μm dust emission polarisation observations of the L1495A-B10 region of the Taurus molecular cloud, taken at the JCMT. We observe a roughly triangular n…

astro-ph.HE2023★ 23 cited

Effective Shielding of 10 GeV Cosmic Rays from Dense Molecular Clumps

Rui-zhi Yang, Guang-Xing Li, Emma de Oña Wilhelmi +3

The density of cosmic rays inside molecular clouds determines the ionization rate in the dense cores where stars form. It is also one of the drivers of astrochemistry leading to th…

astro-ph.GA2023★ 71 cited

ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions -- XV. Steady Accretion from Global Collapse to Core Feeding in Massive Hub-filament System SDC335

Feng-Wei Xu, Ke Wang, Tie Liu +37

We present ALMA Band-3/7 observations towards "the Heart" of a massive hub-filament system (HFS) SDC335, to investigate its fragmentation and accretion. At a resolution of $\sim0.0…