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19942026
most citedOutflow Feedback Regulated Massive Star Formation in Parsec-Scale Cluster Forming Clumps

387 citations · 7.1k across the 144 of their papers we have counts for

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Showing 2020 · astro-ph.GAShow all

11 papers · 2 filters

astro-ph.GA2020★ 84 cited

Dust polarized emission observations of NGC 6334; BISTRO reveals the details of the complex but organized magnetic field structure of the high-mass star-forming hub-filament network

D. Arzoumanian, R. Furuya, T. Hasegawa +145

[Abridged] Filaments and hubs have received special attention recently thanks to studies showing their role in star formation. While the column density and velocity structures of b…

astro-ph.GA2020★ 11 cited

Carbon Chain Chemistry in Hot-Core Regions around Three Massive Young Stellar Objects Associated with 6.7 GHz Methanol Masers

Kotomi Taniguchi, Eric Herbst, Liton Majumdar +7

We have carried out observations of CCH (), CHCN (), and three C isotopologues of HCN () toward three massive young stellar objects (MYSOs)…

astro-ph.GA2020★ 27 cited

Observations of magnetic fields surrounding LkH 101 taken by the BISTRO survey with JCMT-POL-2

Nguyen Bich Ngoc, Pham Ngoc Diep, Harriet Parsons +146

We report the first high spatial resolution measurement of magnetic fields surrounding LkH 101, a part of the Auriga-California molecular cloud. The observations were taken with…

astro-ph.GA2020★ 10 cited

The CARMA-NRO Orion Survey: Filament Formation via Collision-Induced Magnetic Reconnection -- The Stick in Orion A

Shuo Kong, Volker Ossenkopf-Okada, Héctor G. Arce +13

A unique filament is identified in the {\it Herschel} maps of the Orion A giant molecular cloud. The filament, which, we name the Stick, is ruler-straight and at an early evolution…

astro-ph.GA2020★ 62 cited

The ALMA Survey of 70 Dark High-mass Clumps in Early Stages (ASHES). II: Molecular Outflows in the Extreme Early Stages of Protocluster Formation

Shanghuo Li, Patricio Sanhueza, Qizhou Zhang +15

We present a study of outflows at extremely early stages of high-mass star formation obtained from the ALMA Survey of 70 dark High-mass clumps in Early Stages (ASHES). Twe…

astro-ph.GA2020★ 89 cited

Magnetized filamentary gas flows feeding the young embedded cluster in Serpens South

Thushara G. S. Pillai, Dan P. Clemens, Stefan Reissl +11

Observations indicate that molecular clouds are strongly magnetized, and that magnetic fields influence the formation of stars. A key observation supporting the conclusion that mol…

astro-ph.GA2020★ 59 cited

The JCMT BISTRO Survey: Magnetic Fields Associated with a Network of Filaments in NGC 1333

Yasuo Doi, Tetsuo Hasegawa, Ray S. Furuya +135

We present new observations of the active star-formation region NGC 1333 in the Perseus molecular cloud complex from the James Clerk Maxwell Telescope B-Fields In Star-forming Regi…

astro-ph.GA2020★ 8 cited

Cloud structures in M17 SWex : Possible cloud-cloud collision

Shinichi W. Kinoshita, Fumitaka Nakamura, Quang Nguyen-Luong +11

Using wide-field CO () data taken with the Nobeyama 45-m telescope, we investigate cloud structures of the infrared dark cloud complex in M17 with SCIMES. In total, w…

astro-ph.GA2020★ 125 cited

The molecular cloud lifecycle

Mélanie Chevance, J. M. Diederik Kruijssen, Enrique Vazquez-Semadeni +6

Giant molecular clouds (GMCs) and their stellar offspring are the building blocks of galaxies. The physical characteristics of GMCs and their evolution are tightly connected to gal…

astro-ph.GA2020★ 28 cited

The CARMA-NRO Orion Survey: Protostellar Outflows, Energetics, and Filamentary Alignment

Jesse R. Feddersen, Héctor G. Arce, Shuo Kong +7

We identify 45 protostellar outflows in CO maps of the Orion A giant molecular cloud from the CARMA-NRO Orion survey. Our sample includes 11 newly detected outflows. We measure the…

astro-ph.GA2020★ 17 cited

Large-scale molecular gas distribution in the M17 cloud complex: dense gas conditions of massive star formation?

Quang Nguyen-Luong, Fumitaka Nakamura, Koji Sugitani +8

The non-uniform distribution of gas and protostars in molecular clouds is caused by combinations of various physical processes that are difficult to separate. We explore this non-u…