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dc.contributor.authorChrysostomou, A.
dc.contributor.authorBurton, M.
dc.contributor.authorAxon, D.J.
dc.contributor.authorBrand, P.W.J.L.
dc.contributor.authorHough, J.
dc.contributor.authorBland-Hawthorn, J.
dc.contributor.authorGeballe, T.
dc.date.accessioned2008-02-01T11:36:29Z
dc.date.available2008-02-01T11:36:29Z
dc.date.issued1995
dc.identifier.citationChrysostomou , A , Burton , M , Axon , D J , Brand , P W J L , Hough , J , Bland-Hawthorn , J & Geballe , T 1995 , High Resolution Studies of Molecular Hydrogen by Means of Near-Infrared Fabry-Perot Imaging . in In: Procs of Tridimensional Optical Spectroscopic Methods in Astrophysics, ASP Conference Series 71 . Astronomical Society of the Pacific , pp. 173-181 .
dc.identifier.isbn0-937707-90-2
dc.identifier.otherPURE: 168048
dc.identifier.otherPURE UUID: 840b8f6a-e5d7-40bb-8bc4-b268821487e9
dc.identifier.otherdspace: 2299/1515
dc.identifier.urihttp://hdl.handle.net/2299/1515
dc.descriptionOriginal paper can be found at: http://www.astrosociety.org/pubs/cs/070-112.html--Copyright Astronomical Society of the Pacific
dc.description.abstractWe present a study of the velocity profiles of the v=1-0 S(1) transition of molecular hydrogen (H2) towards the star forming region of OMC-1. A three dimensional data cube is presented which displays the spatial distribution as well as the velocity structure of the H2 emission. A brief description of the data acquisition, reduction and analysis is given.en
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofIn: Procs of Tridimensional Optical Spectroscopic Methods in Astrophysics, ASP Conference Series 71
dc.rightsOpen
dc.titleHigh Resolution Studies of Molecular Hydrogen by Means of Near-Infrared Fabry-Perot Imagingen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dcterms.dateAccepted1995
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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