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A new interstellar molecule: triearbon monoxide
Nature, 1984The published version is located at http://www.nature.com/nature/journal/v310/n5973/abs/310125a0 ...
MATTHEWS, HE +4 more
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Interstellar molecule reactions
Reviews of Modern Physics, 1976Considerable progress has been made during the past five years toward a quantitative understanding of the formation and destruction processes for interstellar molecules. Two areas have been most successful---investigations of the formation process for molecular hydrogen on the surfaces of dust grains and studies of reactions involving positive ions in ...
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Molecules in Interstellar Clouds
1981The physical and chemical state of interstellar clouds is reviewed, including recent investigations at the Onsala Space Observatory. The Orion A region is chosen as an example of a “giant” molecular cloud and hence a formation site for massive stars. The Taurus Molecular Clouds, in contrast, may be the future birthplace of solar-type stars.
Irvine, William M. +2 more
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Interstellar Molecules and Interstellar Chemistry
1986Radio astronomers have to date detected some 60 or so molecules in interstellar space. These molecules have been identified, in the majority of cases, by recording the microwave spectrum received by radio telescope from an interstellar or circumstellar dust cloud and comparing it with the spectra produced in laboratory experiments.
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Interstellar Molecules and Astrochemistry
1988The quantitative study of the interstellar medium (ISM) began with Hartman’s detection in 1904 of the resonance lines of Ca and K, seen in absorption against bright stars by intervening diffuse clouds. Other atoms (Na,Fe,Ti) were subsequently detected, although the overwhelming abundance of H was not recognized until the 1930s.
Barry E. Turner, Lucy M. Ziurys
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