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20102024
most citedFilamentary Fragmentation and Accretion in High-Mass Star-Forming Molecular Clouds

116 citations · 531 across the 15 of their papers we have counts for

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12 papers · 1 filter

astro-ph.GA2024

INvestigations of massive Filaments ANd sTar formation (INFANT). I. Core Identification and Core Mass Function

Yu Cheng, Xing Lu, Patricio Sanhueza +16

Filamentary structures are ubiquitously found in high-mass star-forming clouds. To investigate the relationship between filaments and star formation, we carry out the INFANT (INves…

astro-ph.GA2022★ 29 cited

The ALMA Survey of 70 μm Dark High-mass Clumps in Early Stages (ASHES). VI. The core-scale CO-depletion

Giovanni Sabatini, Stefano Bovino, Patricio Sanhueza +11

Studying the physical and chemical properties of cold and dense molecular clouds is crucial for the understanding of how stars form. Under the typical conditions of infrared dark c…

astro-ph.GA2021★ 32 cited

ALMA observations of NGC 6334S. II. Subsonic and Transonic Narrow Filaments in a High-mass Star Formation Cloud

Shanghuo Li, Patricio Sanhueza, Chang Won Lee +22

We present a study of narrow filaments toward a massive infrared dark cloud, NGC 6334S, using the Atacama Large Millimeter/submillimeter Array (ALMA). Thirteen gas filaments are id…

astro-ph.GA2021★ 41 cited

The ALMA Survey of 70 m Dark High-mass Clumps in Early Stages (ASHES). IV. Star formation signatures in G023.477

Kaho Morii, Patricio Sanhueza, Fumitaka Nakamura +15

With a mass of 1000 and a surface density of 0.5 g cm, G023.477+0.114 also known as IRDC 18310-4 is an infrared dark cloud (IRDC) that has the potentia…

astro-ph.GA2021★ 13 cited

Molecular Cloud Cores with High Deuterium Fractions: Nobeyama Mapping Survey

Ken'ichi Tatematsu, Gwanjeong Kim, Tie Liu +35

We present the results of on-the-fly mapping observations of 44 fields containing 107 SCUBA-2 cores in the emission lines of molecules, NH, HCN, and CCS at 8294 GHz…

astro-ph.GA2018★ 37 cited

Magnetic fields at the onset of high-mass star formation

H. Beuther, J. Soler, W. Vlemmings +9

Context: The importance of magnetic fields at the onset of star formation related to the early fragmentation and collapse processes is largely unexplored today. Aims: We want to un…

astro-ph.GA2018★ 116 cited

Filamentary Fragmentation and Accretion in High-Mass Star-Forming Molecular Clouds

Xing Lu, Qizhou Zhang, Hauyu Baobab Liu +7

Filamentary structures are ubiquitous in high-mass star-forming molecular clouds. Their relation with high-mass star formation is still to be understood. Here we report interferome…

astro-ph.GA2017★ 69 cited

The TOP-SCOPE survey of Planck Galactic Cold Clumps: Survey overview and results of an exemplar source, PGCC G26.53+0.17

Tie Liu, Kee-Tae Kim, Mika Juvela +11

The low dust temperatures (<14 K) of Planck Galactic Cold Clumps (PGCCs) make them ideal targets to probe the initial conditions and very early phase of star formation. TOP-SCOPE i…

astro-ph.GA2016★ 21 cited

Inferring the evolutionary stages of the internal structures of NGC 7538 S and IRS1 from chemistry

S. Feng, H. Beuther, D. Semenov +4

To unambiguously diagnose the detailed physical mechanisms and the evolutionary status of high-mass star-forming regions (HMSFRs), we have performed 0.4" ( AU) resolution…

astro-ph.GA2016★ 44 cited

Outflow detection in a 70 m dark high-mass core

S. Feng, H. Beuther, Q. Zhang +4

We present observations towards a high-mass (), low luminosity () m dark molecular core G 28.34 S-A at 3.4 mm, using the IRAM 30…

astro-ph.GA2016★ 40 cited

Are Infrared Dark Clouds Really Quiescent?

S. Feng, H. Beuther, Q. Zhang +4

The dense, cold regions where high-mass stars form are poorly characterised, yet they represent an ideal opportunity to learn more about the initial conditions of high-mass star fo…

astro-ph.GA2015★ 51 cited

Hierarchical fragmentation and collapse signatures in a high-mass starless region

H. Beuther, Th. Henning, H. Linz +6

Aims: Understanding the fragmentation and collapse properties of the dense gas during the onset of high-mass star formation. Methods: We observed the massive (~800M_sun) starless g…