The Chemical Structure of Young High-mass Star-forming Clumps. II. Parsec-scale CO Depletion and Deuterium Fraction of HCO+

Please use this identifier to cite or link to this item: http://ir.sinica.edu.tw/handle/201000000A/80495

Title:	The Chemical Structure of Young High-mass Star-forming Clumps. II. Parsec-scale CO Depletion and Deuterium Fraction of HCO+
Authors:	S. Feng 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. Wang Z. Y. Zhang S. Zahorecz G. Li H. B. Liu J. Yuan
Issue Date:	2020-10
Relation:	The Astrophysical Journal 901(2), 145
URI:	http://ir.sinica.edu.tw/handle/201000000A/80495
ISSN:	http://gateway.isiknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=Drexel&SrcApp=hagerty_opac&KeyRecord=0004-637X&DestApp=JCR&RQ=IF_CAT_BOXPLOT
URL:	http://dx.doi.org/10.3847/1538-4357/abada3
Appears in Collections:	天文及天文物理研究所

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