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Extended fine structure and continuum emission from S140/L1204

Emery, R; Aannestad, P; Minchin, N; Unger, SJ; Baluteau, JP; Barlow, MJ; Caux, E; ... Smith, A; + view all (1996) Extended fine structure and continuum emission from S140/L1204. Astronomy & Astrophysics , 315 (2) L285-L288. Green open access

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Abstract

Grating spectra, covering the wavelength range 45 to 187μm have been taken with the ISO Long Wavelength Spectrometer (LWS) at a series of pointing positions over the S 140 region, centred on the cluster of embedded young stellar objects at the south-west corner of the L1204 molecular cloud. Extended emission from [CII]158μm and [OI]63μm is seen, peaking near the position of the embedded stars. The measurements of the fine structure lines are interpreted in terms of PDR models for the emission, as well as the underlying thermal continuum for the heated gas and dust.

Type: Article
Title: Extended fine structure and continuum emission from S140/L1204
Open access status: An open access version is available from UCL Discovery
Publisher version: https://ui.adsabs.harvard.edu/abs/1996A%26A...315L...
Language: English
Additional information: This version is the version of record. For information on re-use, please refer to the publisher’s terms and conditions.
Keywords: Science & Technology, Physical Sciences, Astronomy & Astrophysics, ISM, S140, I-III regions, ISM, clouds, infrared, interstellar, lines, infrared, interstellar, continuum, MOLECULAR CLOUDS, PHOTODISSOCIATION REGIONS, S140, S-140/L-1204, OUTFLOW, CARBON, LINE
UCL classification: UCL
UCL > Provost and Vice Provost Offices
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy
URI: https://discovery.ucl.ac.uk/id/eprint/10096129
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