1993
DOI: 10.1002/mas.1280120503
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Gas‐phase ion‐atom reactions

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Cited by 24 publications
(20 citation statements)
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“…10 and references therein. The reverse reaction CH + + H → C + + H 2 + (0.398 ± 0.003) eV (1) represents an important destruction mechanism of CH + the formation of which is poorly understood in diffuse interstellar molecular clouds. Simple models underestimate the observed abundances and, therefore, it is assumed that shock waves, turbulences or UV radiation must play a role.…”
Section: Ch + + H Ch + + Dmentioning
confidence: 99%
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“…10 and references therein. The reverse reaction CH + + H → C + + H 2 + (0.398 ± 0.003) eV (1) represents an important destruction mechanism of CH + the formation of which is poorly understood in diffuse interstellar molecular clouds. Simple models underestimate the observed abundances and, therefore, it is assumed that shock waves, turbulences or UV radiation must play a role.…”
Section: Ch + + H Ch + + Dmentioning
confidence: 99%
“…With the AB-22PT technique the rate coefficient for reaction (1) has been determined at 50 K and 100 K. For T H = T ion = 50 K a rate coefficient of 1.3 × 10 -9 cm 3 s -1 has been obtained. At an accommodator temperature of 100 K and a trap temperature of 80 K, a value of 8.7 × 10 -10 cm 3 s -1 has been measured.…”
Section: Ch + + H Ch + + Dmentioning
confidence: 99%
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“…There are several reports on the interactions between thermal H . radicals and various ions, as probed by mass spectrometry 11–17. In these studies, a microwave discharge in H 2 or hydrocarbon gases has been the sole method for generation of H .…”
mentioning
confidence: 99%
“…Investigating the properties of reactions that take place in naturally-occurring cold environments is necessary in order to accurately model their chemistry. [1][2][3][4][5][6][7][8][9][10] Even now, many of the reactions postulated to be of astrochemical importance are yet to be experimentally measured under cold conditions.…”
Section: Introductionmentioning
confidence: 99%