Warm neutral halos around molecular clouds. V - OH (1665 and 1667 MHz) observations

Ten strip maps of 1665- and 1667-MHz OH emission, traversing the outer boundaries of five molecular clouds, were made. The OH emission is found to be significantly extended relative to CO, from which it inferred that OH is to be found in abundance in the shell of partly atomic, partly molecular gas...

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Veröffentlicht in:The Astrophysical journal 1993-04, Vol.407 (1), p.163-174
Hauptverfasser: Wannier, Peter G., Andersson, B.-G., Federman, S. R., Lewis, B. M., Viala, Y. P., Shaya, E.
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container_end_page 174
container_issue 1
container_start_page 163
container_title The Astrophysical journal
container_volume 407
creator Wannier, Peter G.
Andersson, B.-G.
Federman, S. R.
Lewis, B. M.
Viala, Y. P.
Shaya, E.
description Ten strip maps of 1665- and 1667-MHz OH emission, traversing the outer boundaries of five molecular clouds, were made. The OH emission is found to be significantly extended relative to CO, from which it inferred that OH is to be found in abundance in the shell of partly atomic, partly molecular gas surrounding the dense molecular clouds. The fractional OH abundance is calculated using existing H I and CO observations, and detailed source models which include a complete chemistry network and a radiative transfer code. It is concluded that the extended OH is formed, not by the exothermic reaction of O with H3(+), but by the endothermic reaction, H(+) + O yields H + O(+).
doi_str_mv 10.1086/172502
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source NASA Technical Reports Server; Alma/SFX Local Collection
subjects Astronomy
Astrophysics
Atomic, molecular, chemical, and grain processes
Earth, ocean, space
Exact sciences and technology
Interstellar medium (ism) and nebulae in milky way
Molecular clouds, h2 clouds, dense clouds, and dark clouds
Stellar systems. Galactic and extragalactic objects and systems. The universe
title Warm neutral halos around molecular clouds. V - OH (1665 and 1667 MHz) observations
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