Aperture synthesis observations of NH3 in OMC-1 - Filamentary structures around Orion-KL

Astronomy and Astrophysics – Astrophysics

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Ammonia, Herbig-Haro Objects, Molecular Clouds, Orion Nebula, Pre-Main Sequence Stars, Rotational Spectra, Astronomical Maps, Hydrogen, Stellar Winds, Synthetic Apertures

Scientific paper

Aperture synthesis observations of the Orion molecular cloud 1 (OMC-1) have been made in NH3 (1, 1) and (2, 2) emission at 23.7 GHz, using the Nobeyama Millimeter Array (NMA), and obtained 16 arcsec resolution maps for OMC-1 and 8 arcsec resolution maps for the Orion-KL region. Filamentary structures extending over 0.5 pc from the Orion-KL region to the north and northwest directions were found. These structures are associated with the H2 finger structures and Herbig-Haro objects which are located at the blue-shifted side of the bipolar molecular outflow. The results suggest that these filaments are ambient molecular cloudlets with shocked surfaces caused by the strong stellar wind from the Orion-KL region. The 8 arcsec resolution NH3 (2, 2) maps show the extended features around the hot core of Orion-KL. These extended features correspond to the rotating disk and shocked shell associated with the bipolar molecular outflow.

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