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ISO-LWS grating spectroscopy: the case of R CrA star forming region

Giannini, T.; Lorenzotti, D.; Benedettini, M.; Nisini, B.; Saraceno, P.; Tommasi, E.; Smith, H. A. and White, G. J. (1998). ISO-LWS grating spectroscopy: the case of R CrA star forming region. In: Star Formation with the Infrared Space Observatory, 24-26 June 1997, Lisbon, Portugal.

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Abstract

We present the far infrared spectra of the R CrA star forming region obtained with ISO-LWS. We collected a pointed observation on the Herbig Ae star R CrA and a raster scan covering the surrounding region, where HH100 (with its exciting source) and the pre-Main Sequence star T CrA are located. The OI 63μm and the CII 158μm lines have been detected in all the pointed positions, with a ratio consistent with PDR excitation. CO rotational lines (between Jup=14 and Jup=19) are detected on R CrA; from their intensities we derived, using a LVG model, the density and temperature of the emitting region. Other molecular transitions (OH and H2O) have been detected on the investigated objects; the derived cooling of all the molecular species is in agreement with C-shock as the likely excitation mechanism. The continuum emission of R CrA peaks around 100μm (as expected for a Herbig star) while the other sources (T CrA, HH100) show increasing continua up to ~200μm, indicating that they are probably less evolved sources.

Item Type: Conference Item
Copyright Holders: 1998 Astronomical Society of the Pacific
Extra Information: Star Formation with the Infrared Space Observatory (ISO)
ASP Conference Series, Vol. 132, 1998
J. L. Yun, and R. Liseau, eds.
Print ISBN: 1-886733-52-X
e-Book ISBN: 978-1-58381-468-0
pp.350-353
Academic Unit/Department: Science > Physical Sciences
Interdisciplinary Research Centre: Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)
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Item ID: 32672
Depositing User: Glenn White
Date Deposited: 16 Mar 2012 09:54
Last Modified: 17 Mar 2012 00:06
URI: http://oro.open.ac.uk/id/eprint/32672
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