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Thomas J Haworth, Jinyoung S Kim, Andrew J Winter, et al. Monthly Notices of the Royal Astronomical Society 501(3) 3502 (2021) https://doi.org/10.1093/mnras/staa3918
C18O,13CO, and12CO abundances and excitation temperatures in the Orion B molecular cloud
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The JCMT BISTRO Survey: Alignment between Outflows and Magnetic Fields in Dense Cores/Clumps
Hsi-Wei Yen, Patrick M. Koch, Charles L. H. Hull, Derek Ward-Thompson, Pierre Bastien, Tetsuo Hasegawa, Woojin Kwon, Shih-Ping Lai, Keping Qiu, Tao-Chung Ching, Eun Jung Chung, Simon Coudé, James Di Francesco, Pham Ngoc Diep, Yasuo Doi, Chakali Eswaraiah, Sam Falle, Gary Fuller, Ray S. Furuya, Ilseung Han, Jennifer Hatchell, Martin Houde, Shu-ichiro Inutsuka, Doug Johnstone, Ji-hyun Kang, et al. The Astrophysical Journal 907(1) 33 (2021) https://doi.org/10.3847/1538-4357/abca99
Testing the models of X-ray driven photoevaporation with accreting stars in the Orion Nebula Cluster
Wanggi Lim, Fumitaka Nakamura, Benjamin Wu, Thomas G Bisbas, Jonathan C Tan, Edward Chambers, John Bally, Shuo Kong, Peregrine McGehee, Dariusz C Lis, Volker Ossenkopf-Okada and Álvaro Sánchez-Monge Publications of the Astronomical Society of Japan 73(Supplement_1) S239 (2021) https://doi.org/10.1093/pasj/psaa035
Symmetry properties and widths of the filamentary structures in the Orion A giant molecular cloud
Maria S Murga, Maria S Kirsanova, Dmitry S Wiebe and Paul A Boley Monthly Notices of the Royal Astronomical Society 509(1) 800 (2021) https://doi.org/10.1093/mnras/stab3061
A VLBA Survey of Radio Stars in the Orion Nebula Cluster. I. The Nonthermal Radio Population
A kinematic analysis of the CO clouds toward a reflection nebula NGC 2023 observed using the Nobeyama 45 m telescope: Further evidence for a cloud–cloud collision in the Orion region
Rin I Yamada, Rei Enokiya, Hidetoshi Sano, Shinji Fujita, Mikito Kohno, Daichi Tsutsumi, Atsushi Nishimura, Kengo Tachihara and Yasuo Fukui Publications of the Astronomical Society of Japan 73(4) 880 (2021) https://doi.org/10.1093/pasj/psab050
The Explosion in Orion-KL as Seen by Mosaicking the Magnetic Field with ALMA
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Tracing PAH Size in Prominent Nearby Mid-Infrared Environments