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2020ApJ...901..145F - Astrophys. J., 901, 145-145 (2020/October-1)
The chemical structure of young high-mass star-forming clumps. II. Parsec-scale CO depletion and deuterium fraction of HCO+.
FENG S., LI D., CASELLI P., DU F., LIN Y., SIPILA O., BEUTHER H., SANHUEZA P., TATEMATSU K., LIU S.Y., ZHANG Q., WANG Y., HOGGE T., JIMENEZ-SERRA I., LU X., LIU T., WANG K., ZHANG Z.Y., ZAHORECZ S., LI G., LIU H.B. and YUAN J.
Abstract (from CDS):
Abstract Copyright: © 2020. The American Astronomical Society. All rights reserved.
Journal keyword(s): Interstellar medium - Interstellar molecules - Star formation - Massive stars - Astrochemistry
Nomenclature: Fig. 1, Table 2: [FLC2020] GLLL.ll+BB.bb PN N=12.
Simbad objects: 39
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