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Distortion of Magnetic Fields in a Starless Core II: 3D Magnetic Field Structure of FeSt 1-457

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Not so different after all: properties and spatial structure of column density peaks in the pipe and Orion A clouds

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DOI: 10.1093/mnras/stz2355
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Primordial mass and density segregation in a young molecular cloud

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What is the physics behind the Larson mass–size relation?

J Ballesteros-Paredes, C Román-Zúñiga, Q Salomé, M Zamora-Avilés and M J Jiménez-Donaire
Monthly Notices of the Royal Astronomical Society 490 (2) 2648 (2019)
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A correlation between chemistry, polarization, and dust properties in the Pipe nebula starless core FeSt 1-457

Carmen Juárez, Josep M. Girart, Pau Frau, et al.
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Prestellar Core Collisions - Impact on the formation of the CMF? A case study on FeSt 1-457

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Proceedings of the International Astronomical Union 14 (S345) 328 (2018)
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Distortion of Magnetic Fields in a Starless Core. VI. Application of Flux Freezing Model and Core Formation of FeSt 1–457

Ryo Kandori, Kohji Tomisaka, Masao Saito, et al.
The Astrophysical Journal 888 (2) 120 (2020)
DOI: 10.3847/1538-4357/ab6081
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