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The chemical composition of interstellar molecular clouds

descriptionPublicationkeyboard_double_arrow_right Article 01 Jan 1984Embargo end date: 26 Apr 2024 United States English Publisher:Springer Science and Business Media LLCJournal:Origins of Life, volume 14, pages 15-23 (issn: 0302-1688, eissn: 1573-0875,

Authors: Irvine, William M.; HJALMARSON, A;

doi: 10.1007/bf00933635 , 10.7275/2426

pmid: 11536582

The chemical composition of interstellar molecular clouds

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Abstract

Relative abundances for molecules observed by radio astronomical techniques have been determined for several interstellar regions with differing physical properties.

The published version is located at http://www.springerlink.com/content/w327411847532321/

Country

United States

Related Organizations

University of Massachusetts System
United States
University of Massachusetts Amherst
United States

Keywords

Carbon Monoxide, Astrophysics and Astronomy, Evolution, Chemical, Extraterrestrial Environment, Astronomy, Spectrum Analysis, astrobiology, Interstellar Medium and the Galaxy, Stars, Hydrogen Cyanide, Nitriles, Interstellar Chemistry, Gases, Hydrogen

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	citations This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	18
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	influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	Top 10%
	impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.	Average