Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2277
Title: Mapping of the Orion molecular cloud in the [CII] line and continuum at 158 μm
Authors: Mookerjea, B
Ghosh, S. K
Kaneda, H
Nakagawa, T
Ojha, D. K
Rengarajan, T. N
Shibai, H
Verma, R. P
Keywords: Orion;Molecular cloud;Continuum
Issue Date: 2001
Publisher: Astronomical Society of India
Citation: BASI, Vol. 29, No. 3, pp. 337 - 338
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.
URI: http://hdl.handle.net/2248/2277
???metadata.dc.relation.uri???: http://adsabs.harvard.edu/abs/2001BASI...29..337M
Appears in Collections:BASI Publications

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