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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2277
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dc.contributor.authorMookerjea, B-
dc.contributor.authorGhosh, S. K-
dc.contributor.authorKaneda, H-
dc.contributor.authorNakagawa, T-
dc.contributor.authorOjha, D. K-
dc.contributor.authorRengarajan, T. N-
dc.contributor.authorShibai, H-
dc.contributor.authorVerma, R. P-
dc.date.accessioned2008-05-08T11:03:13Z-
dc.date.available2008-05-08T11:03:13Z-
dc.date.issued2001-
dc.identifier.citationBASI, Vol. 29, No. 3, pp. 337 - 338en
dc.identifier.urihttp://hdl.handle.net/2248/2277-
dc.description.abstractA fabry Perot Spectrometer (FPS) tuned to the astrophysically interesting (CII) line at 157.7409 µm, developed at ISAS (Japan) has been successfully interfaced to the TIFR 100 cm far-infrared balloon borne telescope. A region (30' x 15') of the Orion molecular cloud was mapped with a spectral resolution of 1700 and angular resolution of ~ 1'. The spatial distribution of (CII) line emission at 157.7409 µm and the neighboring dust continuum are presented here.en
dc.format.extent169676 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2001BASI...29..337Men
dc.subjectOrionen
dc.subjectMolecular clouden
dc.subjectContinuumen
dc.titleMapping of the Orion molecular cloud in the [CII] line and continuum at 158 μmen
dc.typeArticleen
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