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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1556
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dc.contributor.authorSeema, P-
dc.contributor.authorBanerjee, D. P. K-
dc.contributor.authorAnandarao, B. G-
dc.date.accessioned2007-05-09T08:32:45Z-
dc.date.available2007-05-09T08:32:45Z-
dc.date.issued1993-
dc.identifier.citationBASI, Vol. 21, pp. 569-573en
dc.identifier.urihttp://hdl.handle.net/2248/1556-
dc.description.abstractHigh quality interferograms have been obtained on the H II region in the Orion Nebula in the emission line of (OIII) 5007 A using the high resolution imaging Fabry-Perot spectrometer. Velocity profiles were obtained for about 2000 spatial positions. Two velocity components, a narrow one with full width at half maximum (FWHM) of around 20 +/- 3 km/sec and a broad one with FWHM of around 50 +/- 3 km/sec are predominantly present in the profiles across the nebulaen
dc.format.extent364261 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectOrion nebulaen
dc.subjectVelocity structureen
dc.titleVelocity field structure in the Orion Nebulaen
dc.typeArticleen
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