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A study of HCN, HNC and their isotopometers in OMC-1. I. Abundances and chemistry.

P. Schilke, C. Malcolm Walmsley, G. Pineau des Forêts, E. Roueff, David R. Flower, S. Guilloteau

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Abstract

We present observations of HCN, HNC, and their isotopically substituted variants towards the Orion hot core and ridge. We used mainly the IRAM 30-m dish with an angular resolution of typically 25″, but we have also made a map of the HC 15 N(J=1-0) transition using the Plateau de Bure Interferometer with an angular resolution of 4″. We determined the HCN, HNC and DCN abundances and estimated density and kinetic temperature at seventeen selected positions in OMC-1.

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What this paper is about

We present observations of HCN, HNC, and their isotopically substituted variants towards the Orion hot core and ridge. We used mainly the IRAM 30-m dish with an angular resolution of typically 25″, but we have also made a map of the HC 15 N(J=1-0) transition using the Plateau de Bure Interferometer with an angular resolution of 4″. We determined the HCN, HNC and DCN abundances and estimated density and kinetic temperature at seventeen selected positions in OMC-1.

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Available abstract

We present observations of HCN, HNC, and their isotopically substituted variants towards the Orion hot core and ridge. We used mainly the IRAM 30-m dish with an angular resolution of typically 25″, but we have also made a map of the HC 15 N(J=1-0) transition using the Plateau de Bure Interferometer with an angular resolution of 4″. We determined the HCN, HNC and DCN abundances and estimated density and kinetic temperature at seventeen selected positions in OMC-1.

Key concepts: Plateau de Bure Interferometer, Physics, Astrophysics, Ridge, Astrochemistry, Angular resolution (graph drawing), Plateau (mathematics), Resolution (logic)

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