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IPA: Class 0 Protostars Viewed in CO Emission Using JWST

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Far-infrared line emission from the outer Galaxy cluster Gy 3–7 with SOFIA/FIFI-LS: Physical conditions and UV fields

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Velocity-resolved high-J CO emission from massive star-forming clumps

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Importance of radiative pumping for the excitation of the H2O submillimeter lines in galaxies

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Astronomy & Astrophysics 666 L3 (2022)
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Water in star-forming regions: physics and chemistry from clouds to disks as probed by Herschel spectroscopy

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CO in Protostars (COPS): Herschel-SPIRE Spectroscopy of Embedded Protostars∗

Yao-Lun Yang, Joel D. Green, Neal J. Evans II, Jeong-Eun Lee, Jes K. Jørgensen, Lars E. Kristensen, Joseph C. Mottram, Gregory Herczeg, Agata Karska, Odysseas Dionatos, Edwin A. Bergin, Jeroen Bouwman, Ewine F. van Dishoeck, Tim A. van Kempen, Rebecca L. Larson and Umut A. Yıldız
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The Herschel-PACS Legacy of Low-mass Protostars: The Properties of Warm and Hot Gas Components and Their Origin in Far-UV Illuminated Shocks

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Outflows, infall and evolution of a sample of embedded low-mass protostars

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Origin of warm and hot gas emission from low-mass protostars: Herschel-HIFI observations of CO J = 16–15

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THE EVOLUTION OF FAR-INFRARED CO EMISSION FROM PROTOSTARS

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https://doi.org/10.3847/0004-637X/831/1/69