A 3D view of the outflow in the Orion Molecular Cloud 1 (OMC-1)
Open Access
- 9 April 2012
- journal article
- research article
- Published by EDP Sciences in Astronomy & Astrophysics
- Vol. 540, A119
Abstract
Context. Stars whose mass is an order of magnitude greater than the Sun play a prominent role in the evolution of galaxies, exploding as supernovae, triggering bursts of star formation and spreading heavy elements about their host galaxies. A fundamental aspect of star formation is the creation of an outflow. The fast outflow emerging from a region associated with massive star formation in the Orion Molecular Cloud 1 (OMC-1), located behind the Orion Nebula, appears to have been set in motion by an explosive event.Aims. We study the structure and dynamics of outflows in OMC-1. We combine radial velocity and proper motion data for near-IR emission of molecular hydrogen to obtain the first 3-dimensional (3D) structure of the OMC-1 outflow. Our work illustrates a new diagnostic tool for studies of star formation that will be exploited in the near future with the advent of high spatial resolution spectro-imaging in particular with data from the Atacama Large Millimeter Array (ALMA).Methods. We used published radial and proper motion velocities obtained from the shock-excited vibrational emission in the H2 v = 1−0 S(1) line at 2.122 μm obtained with the GriF instrument on the Canada-France-Hawaii Telescope, the Apache Point Observatory, the Anglo-Australian Observatory, and the Subaru Telescope.Results. These data give the 3D velocity of ejecta yielding a 3D reconstruction of the outflows. This allows one to view the material from different vantage points in space giving considerable insight into the geometry. Our analysis indicates that the ejection occurred ≲720 years ago from a distorted ring-like structure of ~15″ (6000 AU) in diameter centered on the proposed point of close encounter of the stars BN, source I and maybe also source n. We propose a simple model involving curvature of shock trajectories in magnetic fields through which the origin of the explosion and the center defined by extrapolated proper motions of BN, I and n may be brought into spatial coincidence.Keywords
All Related Versions
This publication has 69 references indexed in Scilit:
- EXPLOSIVE OUTFLOWS POWERED BY THE DECAY OF NON-HIERARCHICAL MULTIPLE SYSTEMS OF MASSIVE STARS: ORION BN/KLThe Astrophysical Journal, 2011
- Identifying the Outflow Driving Sources in Orion-KLThe Astrophysical Journal, 2008
- Outflows and Jets from Collapsing Magnetized Cloud CoresThe Astrophysical Journal, 2006
- Submillimeter Array 440 μm/690 GHz Line and Continuum Observations of Orion KLThe Astrophysical Journal, 2006
- First Detection of28Si18O Maser and Thermal Emission from Orion KLThe Astrophysical Journal, 2005
- On the magnetic acceleration and collimation of astrophysical outflowsMonthly Notices of the Royal Astronomical Society, 1999
- A λ = 1.3 Millimeter Aperture Synthesis Molecular Line Survey of Orion Kleinmann-LowThe Astrophysical Journal, 1996
- High-Resolution CO Observations of the Molecular Outflow in the Orion IRc2 RegionThe Astrophysical Journal, 1996
- Explosive ejection of matter associated with star formation in the Orion nebulaNature, 1993
- Observations of the molecular hydrogen emission from the Orion NebulaThe Astrophysical Journal, 1978