Mapping of the Orion molecular cloud in the [CII] line and continuum at 158 μm

dc.contributor.author	Mookerjea, B
dc.contributor.author	Ghosh, S. K
dc.contributor.author	Kaneda, H
dc.contributor.author	Nakagawa, T
dc.contributor.author	Ojha, D. K
dc.contributor.author	Rengarajan, T. N
dc.contributor.author	Shibai, H
dc.contributor.author	Verma, R. P
dc.date.accessioned	2008-05-08T11:03:13Z
dc.date.available	2008-05-08T11:03:13Z
dc.date.issued	2001
dc.identifier.citation	BASI, Vol. 29, No. 3, pp. 337 - 338	en
dc.identifier.uri	http://hdl.handle.net/2248/2277
dc.description.abstract	A 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.extent	169676 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2001BASI...29..337M	en
dc.subject	Orion	en
dc.subject	Molecular cloud	en
dc.subject	Continuum	en
dc.title	Mapping of the Orion molecular cloud in the [CII] line and continuum at 158 μm	en
dc.type	Article	en