HST emission line images of the Orion HII region: proper motions and possible variability
The Orion Nebula (NGC 1976, M42) contains the nearest massive star forming region and is therefore ideal for studying the physical process accompanying star formation. The high spatial resolution available with HST imaging in emission lines and continuum permits highly detailed study of such processes, as has been described notably by O'Dell (2001)
Gutiérrez, Leonel et al.
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2007