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.
Créditos:International Gemini Observatory/NOIRLab/NSF/AURA
About the Image
Id: | geminiann15004a |
Tipo: | Collage |
Release date: | 12 de Marzo de 2015 a las 12:31 |
Related announcements: | geminiann15004 |
Size: | 500 x 603 px |
Sobre el Objeto
Categoría: | Solar System |