Orion’s Fingers: New Clarity on an Explosive Outflow
A wide-field image showing the OMC1 outflow in H2 with proper motions of the BN object, radio source I, and radio source n superimposed. The lengths of the red-solid vectors are proportional to the motions measured by Gomez et al. (2008) with the the lengths of the vectors in arcseconds equal to the motion in km s-1 (e.g. 1000 corresponds to a motion of 10 km s-1). The ejection center as determined by radio proper motions is shown by a cross.
Credit:International Gemini Observatory/NOIRLab/NSF/AURA
About the Image
Id: | geminiann15004a |
Type: | Collage |
Release date: | March 12, 2015, 12:31 p.m. |
Related announcements: | geminiann15004 |
Size: | 500 x 603 px |
About the Object
Category: | Solar System |