Saraceno, P.; Ceccarelli, C.; Clegg, P.; Correia, C.; di Giorgio, A.; Giannini, T.; Griffin, M.; Lorenzetti, D.; Molinari, S.; Nguyen-Q-Rieu, N; Nisini, B.; Radicchi, A.; Spinoglio, L.; Tommasi, E.; White, G. J.; Ade, P. A. R.; Andre, P.; Armand, C.; Barlow, M. J.; Burgdorf, M.; Caux, E.; Cerulli, P.; Fischer, J.; Furniss, I.; Glencross, B.; Gry, C.; King, K. J.; Lim, T.; Liseau, R.; Minchin, N.; Naylor, D.; Texier, D.; Orfei, R.; Palla, F.; Sidher, S.; Smith, H. A.; Swinyard, B.; Trams, N. and Unger, S.
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We present the first far-infrared spectrum of the IRAS source associated with IC 1396N, located in the HII region IC 1396 together with submillimeter and millimeter photometry. A rich spectrum of CO, OH, and H2O lines are detected in the ISO-LWS spectrum, indicative of a warm, dense region, probably shock excited, around the source. Among the fine structure lines, [OIII] and [NIII] are also detected and can be explained by the presence of the O6 star HD206267 approximately 16pc away.
The far infrared and submillimeter spectral energy distribution is fitted with a model assuming spherical grey-bodies with a radial power law of density and temperature. An accurate measure of the bolometric luminosity and an estimate of the total envelope mass are obtained.
|Item Type:||Journal Article|
|Copyright Holders:||1996 European Southern Observatory|
|Keywords:||stellar formation; jets and outflows; IC 1396N; infrared; lines|
|Academic Unit/Department:||Science > Physical Sciences
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||G. J. White|
|Date Deposited:||22 Mar 2012 11:48|
|Last Modified:||23 Feb 2016 23:00|
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