Gravitational collapse of the OMC-1 region

Abstract

We have investigated the global dynamical state of the Integral Shaped Filament in the Orion A cloud using new N${}_2$H${}^{+}$ (1-0) large-scale, IRAM30m observations. Our analysis of its internal gas dynamics reveals the presence of accelerated motions towards the Orion Nebula Cluster, showing a characteristic blue-shifted profile centred at the position of the OMC-1 South region. The properties of these observed gas motions (profile, extension, and magnitude) are consistent with the expected accelerations for the gravitational collapse of the OMC-1 region and explain both the physical and kinematic structure of this cloud.

arXiv comment5 pages, 2 figures; Accepted by A&A

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