A self-consistent dynamical model of the Milky Way disc adjusted to Gaia data
Robin, A. C. et al., 2022 A&A 667, A98
https://ui.adsabs.harvard.edu/abs/2022A%26A...667A..98R/abstract
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The Lognormal Probability Distribution Function of the Perseus Molecular Cloud: A Comparison of HI and Dust
Burkhar, B, et al., 2015 ApJ Letters, 811,L28
https://ui.adsabs.harvard.edu/abs/2015ApJ...811L..28B/abstract
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Can Turbulent, High-density Gas Form Stars in Molecular Clouds: A Case Study in Ophiuchus
Jiao, S, et al., 2022 A&A 22:075016
https://ui.adsabs.harvard.edu/abs/2022RAA....22g5016J/abstract
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The JCMT Gould Belt Survey: radiative heating by OB stars
Rumble, D., et al., 2021 MNRAS 505,2103‒2110
https://ui.adsabs.harvard.edu/abs/2021MNRAS.505.2103R/abstract
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ALMA-IMF VI. Investigating the origin of stellar masses: Core mass function evolution in the W43-MM2&MM3 mini-starburst
Pouteau, Y, et al., 2022 A&A 674, A76
https://ui.adsabs.harvard.edu/abs/2023A%26A...674A..76P/abstract
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The Molecular Clouds in a Section of the Third Galactic Quadrant: Observational Properties and Chemical Abundance Ratio between CO and its Isotopologues
Wang, C, et al., 2023 ApJ 166,121
https://ui.adsabs.harvard.edu/abs/2023AJ....166..121W/abstract
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Constraining the H2 column densities in the diffuse interstellar medium using dust extinction and HI data
Raphael, S, et al., 2023 arXiv:2312.02274
https://ui.adsabs.harvard.edu/abs/2023arXiv231202274S/abstract
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