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Physicochemical models: source-tailored or generic?
Beatrice M Kulterer, Maria N Drozdovskaya, Audrey Coutens, Sébastien Manigand and Gwendoline Stéphan Monthly Notices of the Royal Astronomical Society 498(1) 276 (2020) https://doi.org/10.1093/mnras/staa2443
Characterizing young protostellar disks with the CALYPSO IRAM-PdBI survey: large Class 0 disks are rare
Chronology of Episodic Accretion in Protostars—An ALMA Survey of the CO and H2O Snowlines
Tien-Hao Hsieh, Nadia M. Murillo, Arnaud Belloche, Naomi Hirano, Catherine Walsh, Ewine F. van Dishoeck, Jes K. Jørgensen and Shih-Ping Lai The Astrophysical Journal 884(2) 149 (2019) https://doi.org/10.3847/1538-4357/ab425a
Role of environment and gas temperature in the formation of multiple protostellar systems: molecular tracers
SIGNS OF EARLY-STAGE DISK GROWTH REVEALED WITH ALMA
Hsi-Wei Yen, Patrick M. Koch, Shigehisa Takakuwa, Ruben Krasnopolsky, Nagayoshi Ohashi and Yusuke Aso The Astrophysical Journal 834(2) 178 (2017) https://doi.org/10.3847/1538-4357/834/2/178
Kinematics of a Young Low-mass Star-forming Core: Understanding the Evolutionary State of the First-core Candidate L1451-mm
María José Maureira, Héctor G. Arce, Michael M. Dunham, Jaime E. Pineda, Manuel Fernández-López, Xuepeng Chen and Diego Mardones The Astrophysical Journal 838(1) 60 (2017) https://doi.org/10.3847/1538-4357/838/1/60
Hot methanol from the inner region of the HH 212 protostellar system
Revealing the dynamics of Class 0 protostellar discs with ALMA
D. Seifried, Á. Sánchez-Monge, S. Walch and R. Banerjee Monthly Notices of the Royal Astronomical Society 459(2) 1892 (2016) https://doi.org/10.1093/mnras/stw785
Constraining the physical structure of the inner few 100 AU scales of deeply embedded low-mass protostars
Small-scale properties of Class 0 protostars from the CALYPSO IRAM-PdBI survey
Anaëlle Maury, Philippe André, Sébastien Maret, et al. Proceedings of the International Astronomical Union 11(S315) 114 (2015) https://doi.org/10.1017/S1743921316007365
OBSERVATIONS OF INFALLING AND ROTATIONAL MOTIONS ON A 1000 AU SCALE AROUND 17 CLASS 0 AND 0/I PROTOSTARS: HINTS OF DISK GROWTH AND MAGNETIC BRAKING?