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dc.contributor.authorRawlings, J.M.C.
dc.contributor.authorDrew, J.E.
dc.contributor.authorBarlow, M.J.
dc.date.accessioned2009-12-01T15:08:22Z
dc.date.available2009-12-01T15:08:22Z
dc.date.issued1993
dc.identifier.citationRawlings , J M C , Drew , J E & Barlow , M J 1993 , ' Excited hydrogen and the formation of molecular-hydrogen via associative ionization. 1 : Physical processes and outflows from young stellar objects ' , Monthly Notices of the Royal Astronomical Society , vol. 265 , no. 4 , pp. 968-982 .
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 154615
dc.identifier.otherPURE UUID: fe8afa97-90e3-43cc-b028-f110d7db533c
dc.identifier.otherdspace: 2299/4051
dc.identifier.urihttp://hdl.handle.net/2299/4051
dc.descriptionOriginal article can be found at: http://adsabs.harvard.edu/basic_search.html Copyright Royal Astronomical Society [Full text of this article is not available in the UHRA]
dc.description.abstractRates for the associative ionization reaction H(n=2)+H→H2++e- are calculated. This reaction is found to be a greater contributor to the H2 formation rate than the direct radiative association reaction H(n=2)+H→H2+hν in most regions of astrophysical interest. Chemical models of circumstellar regions are reassessed in the light of this information. We also examine the chemical behaviour of several other excited chemical species. A critical examination reveals that excitation effects are, in general, very important in many astrophysical situations and must be incorporated into the chemistry. H2 has been detected in a variety of circumstellar regions and has a pivotal role in the overall chemistry. The method and efficiency of its formation are therefore of great importance. We test the significance of the associative ionization reaction in several models. These models include a schematic description of the radiative transfer in H I Lyα. The endothermicity (≃ 1.1 eV) of the reaction and the high departures from LTE that are required for the H I (n=2) level to be sufficiently populated restrict its significance to regions of high excitation, such as are found in circumstellar regions. In this paper (I), we investigate the importance of the reaction in winds associated with young stellar objects. In Paper II, the investigation will be extended to include novae, supernovae, planetary nebulae and shocked regions. The results indicate that reactions involving excited atomic states may be very important in a number of circumstellar chemistries. Only exceptionally will reactions involving the higher excited states (n>2) be as significant as those involving H(n =2).en
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.titleExcited hydrogen and the formation of molecular-hydrogen via associative ionization. 1 : Physical processes and outflows from young stellar objectsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dcterms.dateAccepted1993
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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