Chemical models of interstellar gas-grain processes - III. Molecular depletion in NGC 2024

Monthly Notices of the Royal Astronomical Society

Volumn 291, Issue 3, 1997, Pages 455-460

  Charnley, S B ^a,b  

^a UNIVERSITY OF CALIFORNIA   (United States)

^b NASA AMES RESEARCH CENTER   (United States)

Author keywords

ISM: clouds; ISM: individual: NGC 2024; ISM: molecules; Molecular processes

Indexed keywords

BINDING ENERGY; DENSITY OF GASES; DUST; HEAVY METALS;

CHEMICAL MODEL; COLD DUST; DUST TEMPERATURES; INTERSTELLAR GAS; ISM : CLOUDS; ISM: INDIVIDUAL: NGC 2024; ISM: INDIVIDUALS; ISM:MOLECULES; MOLECULAR PROCESS; ULTRADENSE;

MOLECULES;

EID: 4243223977     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/291.3.455     Document Type: Article

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