Details

Autor(en) / Beteiligte

• Crockett, Nathan R
• Bergin, Edwin A
• Neill, Justin L
• Favre, Cecile
• Schilke, Peter
• Lis, Dariusz C
• Bell, Tom A
• Blake, Geoffrey
• Cernicharo, Jose
• EMPRECHTINGER, MARTIN

Titel

HERSCHEL OBSERVATIONS OF EXTRAORDINARY SOURCES: ANALYSIS OF THE HIFI 1.2 THz WIDE SPECTRAL SURVEY TOWARD ORION KL. I. METHODS

Ist Teil von

• The Astrophysical journal, 2014-06, Vol.787 (2), p.1-35

Ort / Verlag

American Astronomical Society

Erscheinungsjahr

2014

Link zum Volltext

Quelle

Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals

Beschreibungen/Notizen

• We present a comprehensive analysis of a broadband spectral line survey of the Orion Kleinmann-Low nebula (Orion KL), one of the most chemically rich regions in the Galaxy, using the HIFI instrument on board the Herschel Space Observatory. This survey spans a frequency range from 480 to 1907 GHz at a resolution of 1.1 MHz. These observations thus encompass the largest spectral coverage ever obtained toward this high-mass star-forming region in the submillimeter with high spectral resolution and include frequencies > 1 THz, where the Earth's atmosphere prevents observations from the ground. In all, we detect emission from 39 molecules (79 isotopologues). Combining this data set with ground-based millimeter spectroscopy obtained with the IRAM 30 m telescope, we model the molecular emission from the millimeter to the far-IR using the XCLASS program, which assumes local thermodynamic equilibrium (LTE). Several molecules are also modeled with the MADEX non-LTE code. Because of the wide frequency coverage, our models are constrained by transitions over an unprecedented range in excitation energy. A reduced [chi] super(2) analysis indicates that models for most species reproduce the observed emission well. In particular, most complex organics are well fit by LTE implying gas densities are high (>10 super(6) cm super(-3)) and excitation temperatures and column densities are well constrained. Molecular abundances are computed using H sub(2) column densities also derived from the HIFI survey. The distribution of rotation temperatures, T sub(rot), for molecules detected toward the hot core is significantly wider than the compact ridge, plateau, and extended ridge T sub(rot) distributions, indicating the hot core has the most complex thermal structure.