dc.contributor.author | Chrysostomou, A. | |
dc.contributor.author | Burton, M. | |
dc.contributor.author | Axon, D.J. | |
dc.contributor.author | Brand, P.W.J.L. | |
dc.contributor.author | Hough, J. | |
dc.contributor.author | Bland-Hawthorn, J. | |
dc.contributor.author | Geballe, T. | |
dc.date.accessioned | 2008-02-01T11:36:29Z | |
dc.date.available | 2008-02-01T11:36:29Z | |
dc.date.issued | 1995 | |
dc.identifier.citation | Chrysostomou , 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.isbn | 0-937707-90-2 | |
dc.identifier.other | dspace: 2299/1515 | |
dc.identifier.uri | http://hdl.handle.net/2299/1515 | |
dc.description | Original paper can be found at: http://www.astrosociety.org/pubs/cs/070-112.html--Copyright Astronomical Society of the Pacific | |
dc.description.abstract | We 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.format.extent | 641612 | |
dc.language.iso | eng | |
dc.publisher | Astronomical Society of the Pacific | |
dc.relation.ispartof | In: Procs of Tridimensional Optical Spectroscopic Methods in Astrophysics, ASP Conference Series 71 | |
dc.title | High Resolution Studies of Molecular Hydrogen by Means of Near-Infrared Fabry-Perot Imaging | en |
dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
dc.contributor.institution | Centre for Astrophysics Research (CAR) | |
rioxxterms.type | Other | |
herts.preservation.rarelyaccessed | true | |