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The Chemical Structure of Young High-mass Star-forming Clumps. II. Parsec-scale CO Depletion and Deuterium Fraction of HCO+
S. 轶 Feng 冯思, D. Li, P. Caselli, F. Du, Y. Lin, O. Sipilä, H. Beuther, Patricio Sanhueza, K. Tatematsu, S. Y. Liu, Q. Zhang, Y. Wang, T. Hogge, I. Jimenez-Serra, X. Lu, T. Liu, K. 科 Wang 王, Z. Y. Zhang, S. Zahorecz, G. Li, H. B. Liu and J. Yuan The Astrophysical Journal 901(2) 145 (2020) https://doi.org/10.3847/1538-4357/abada3
APEX observations of ortho-H2D+ towards dense cores in the Orion B9 filament
Deuterated forms of H
3
+
and their importance in astrochemistry
P. Caselli, O. Sipilä and J. Harju Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 377(2154) 20180401 (2019) https://doi.org/10.1098/rsta.2018.0401
Modelling the molecular composition and nuclear-spin chemistryof collapsing pre-stellar sources★
P Hily-Blant, A Faure, C Rist, G Pineau des Forêts and D R Flower Monthly Notices of the Royal Astronomical Society 477(4) 4454 (2018) https://doi.org/10.1093/mnras/sty881