84 citations · 908 across the 41 of their papers we have counts for
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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…
Extended HNCO, SiO, and HCN emission in 43 southern star-forming regions
Yu-Xin He, Christian Henkel, Jian-Jun Zhou +9
We have selected 43 southern massive star-forming regions to study the spatial distribution of HNCO 4-3, SiO 2-1 and HCN 10-9 line emission and to investigate t…
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…
Studies of the distinct regions due to CO selective dissociation in the Aquila molecular cloud
Toktarkhan Komesh, Willem Baan, Jarken Esimbek +6
Aims. We investigate the role of selective dissociation in the process of star formation by comparing the physical parameters of protostellar-prestellar cores and the distinct regi…
Ammonia observations towards the Aquila Rift cloud complex
Kadirya Tursun, Jarken Esimbek, Christian Henkel +7
We surveyed the Aquila Rift complex including the Serpens South and W40 region in the NH(1,1) and (2,2) transitions making use of the Nanshan 26-m telescope. The kinetic temper…
Evidence for dense gas heated by the explosion in Orion KL
Dalei Li, Xindi Tang, Christian Henkel +7
We mapped the kinetic temperature structure of Orion KL in a 20 (8000 AU) sized region with para-HCS , , and mak…
NH (1,1) hyperfine intensity anomalies in the Orion A molecular cloud
Dong-dong Zhou, Gang Wu, Jarken Esimbek +5
In LTE, the two inner satellite lines (ISLs) and the two outer satellite lines (OSLs) of the NH (1,1) transition are each predicted to have equal intensities. However, hyperf…