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dc.contributor.authorChrysostomou, A.
dc.contributor.authorBrand, P.W.J.L.
dc.contributor.authorBurton, M.
dc.date.accessioned2008-09-24T09:04:19Z
dc.date.available2008-09-24T09:04:19Z
dc.date.issued1993
dc.identifier.citationChrysostomou , A , Brand , P W J L & Burton , M 1993 , H2 Spectroscopy in the Photodissociation Region of M17 Northern Bar . in In: Astronomical Infrared Spectroscopy: Future Observational Directions - ASP Conf Series 41 . Astronomical Society of the Pacific , pp. 207-210 .
dc.identifier.isbn0-937707-60-0
dc.identifier.isbn978-1-58381-377-5
dc.identifier.otherPURE: 153416
dc.identifier.otherPURE UUID: 6de11c78-76f1-47f7-80dc-e471bb9c813f
dc.identifier.otherdspace: 2299/2392
dc.identifier.urihttp://hdl.handle.net/2299/2392
dc.descriptionOriginal paper can be found at: http://astrosociety.org/pubs/cs/035-069.html Copyright ASP
dc.description.abstractWe present results of long slit spectroscopy, from 2.0 to 2.5 microns, of the photodissociation region in the northern bar of M17. The observations give us an insight into the physical conditions in the region and provide evidence which suggests that the ortho to para ratio of molecular hydrogen does not equal 3. We briefly discuss the astrophysical relevance of this.en
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofIn: Astronomical Infrared Spectroscopy: Future Observational Directions - ASP Conf Series 41
dc.titleH2 Spectroscopy in the Photodissociation Region of M17 Northern Baren
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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