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Herschel observations of EXtra-Ordinary Sources: The Terahertz spectrum of Orion KL seen at high spectral resolution

Authors :
Crockett, N. R.
Bergin, E. A.
Wang, S.
Lis, D. C.
Bell, T. A.
Blake, G. A.
Boogert, A.
Bumble, B.
Cabrit, S.
Caux, E.
Ceccarelli, C.
Cernicharo, J.
Comito, C.
Daniel, F.
Dubernet, M. -L.
Emprechtinger, M.
Encrenaz, P.
Falgarone, E.
Gerin, M.
Giesen, T. F.
Goicoechea, J. R.
Goldsmith, P. F.
Gupta, H.
Gusten, R.
Hartogh, P.
Helmich, F.
Herbst, E.
Honingh, N.
Joblin, C.
Johnstone, D.
Karpov, A.
Kawamura, J. H.
Kooi, J.
Krieg, J. -M.
Langer, W. D.
Latter, W. D.
Lord, S. D.
Maret, S.
Martin, P. G.
Melnick, G. J.
Menten, K. M.
Morris, P.
Muller, H. S. P.
Murphy, J. A.
Neufeld, D. A.
Ossenkopf, V.
Pearson, J. C.
Perault, M.
Phillips, T. G.
Plume, R.
Qin, S. -L.
Roelfsema, P.
Schieder, R.
Schilke, P.
Schlemmer, S.
Stutzki, J.
van der Tak, F. F. S.
Tielens, A.
Trappe, N.
Vastel, C.
Yorke, H. W.
Yu, S.
Zmuidzinas, J.
Publication Year :
2010

Abstract

We present the first high spectral resolution observations of Orion KL in the frequency ranges 1573.4 - 1702.8 GHz (band 6b) and 1788.4 - 1906.8 GHz (band 7b) obtained using the HIFI instrument on board the Herschel Space Observatory. We characterize the main emission lines found in the spectrum, which primarily arise from a range of components associated with Orion KL including the hot core, but also see widespread emission from components associated with molecular outflows traced by H2O, SO2, and OH. We find that the density of observed emission lines is significantly diminished in these bands compared to lower frequency Herschel/HIFI bands.<br />Comment: Accepted for publication in the Herschel HIFI special issue of Astronomy and Astrophysics Letters, 5 pages, 3 figures

Details

Database :
arXiv
Publication Type :
Report
Accession number :
edsarx.1007.4564
Document Type :
Working Paper
Full Text :
https://doi.org/10.1051/0004-6361/201015116