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Theory of Turbulent Equilibrium Spheres with Power-law Linewidth–Size Relation
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Q-band line survey observations toward a carbon-chain-rich clump in the Serpens South region
Kotomi Taniguchi, Fumitaka Nakamura, Sheng-Yuan Liu, Tomomi Shimoikura, Chau-Ching Chiong, Kazuhito Dobashi, Naomi Hirano, Yoshinori Yonekura, Hideko Nomura, Atsushi Nishimura, Hideo Ogawa, Chen Chien, Chin-Ting Ho, Yuh-Jing Hwang, You-Ting Yeh, Shih-Ping Lai, Yasunori Fujii, Yasumasa Yamasaki, Quang Nguyen-Luong and Ryohei Kawabe Publications of the Astronomical Society of Japan 76(6) 1270 (2024) https://doi.org/10.1093/pasj/psae088
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Gas kinematics around filamentary structures in the Orion B cloud
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CMR Exploration. II. Filament Identification with Machine Learning
NEATH – II. N2H+ as a tracer of imminent star formation in quiescent high-density gas
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The Evolution of Protostellar Outflow Cavities, Kinematics, and Angular Distribution of Momentum and Energy in Orion A: Evidence for Dynamical Cores
Cheng-Han 承翰 Hsieh 謝, Héctor G. Arce, Zhi-Yun Li, Michael Dunham, Stella Offner, Ian W. Stephens, Amelia Stutz, Tom Megeath, Shuo Kong, Adele Plunkett, John J. Tobin, Yichen Zhang, Diego Mardones, Jaime E. Pineda, Thomas Stanke and John Carpenter The Astrophysical Journal 947(1) 25 (2023) https://doi.org/10.3847/1538-4357/acba13
Flow of gas detected from beyond the filaments to protostellar scales in Barnard 5
M. T. Valdivia-Mena, J. E. Pineda, D. M. Segura-Cox, P. Caselli, A. Schmiedeke, S. Choudhury, S. S. R. Offner, R. Neri, A. Goodman and G. A. Fuller Astronomy & Astrophysics 677 A92 (2023) https://doi.org/10.1051/0004-6361/202346357
Filaments in the OMC-3 cloud and uncertainties in estimates of filament profiles
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Non-ideal magnetohydrodynamics of self-gravitating filaments
A low-mass hub–filament with double centre revealed in NGC 2071-North
Vera Könyves, D Ward-Thompson, Y Shimajiri, P Palmeirim and Ph André Monthly Notices of the Royal Astronomical Society 520(3) 4646 (2023) https://doi.org/10.1093/mnras/stad132
Stellar Initial Mass Function (IMF) Probed with Supernova Rates and Neutrino Background: Cosmic-average IMF Slope Is ≃2–3 Similar to the Salpeter IMF
Extension of HOPS out to 500 pc (eHOPS). I. Identification and Modeling of Protostars in the Aquila Molecular Clouds*
Riwaj Pokhrel, S. Thomas Megeath, Robert A. Gutermuth, Elise Furlan, William J. Fischer, Samuel Federman, John J. Tobin, Amelia M. Stutz, Lee Hartmann, Mayra Osorio, Dan M. Watson, Thomas Stanke, P. Manoj, Mayank Narang, Prabhani Atnagulov, Nolan Habel and Wafa Zakri The Astrophysical Journal Supplement Series 266(2) 32 (2023) https://doi.org/10.3847/1538-4365/acbfac
Multilognormal density structure in Cygnus-X molecular clouds: a fitting for N-PDF without power law
Takeru Murase, Toshihiro Handa, Ren Matsusaka, et al. Monthly Notices of the Royal Astronomical Society 523(1) 1373 (2023) https://doi.org/10.1093/mnras/stad1451
ALMA-IMF. VIII. Combination of Interferometric Continuum Images with Single-dish Surveys and Structural Analysis of Six Protoclusters
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Simulation of Head-on Collisions between Filamentary Molecular Clouds Threaded by a Lateral Magnetic Field and Subsequent Evolution
Alignment of dense molecular core morphology and velocity gradients with ambient magnetic fields
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