Fig. 1: Radio emission from neutral hydrogen atoms in the direction of the Orion Nebula, the most nearby regions of high-mass star formation. (IMAGE)

University of Vienna

Fig. 1: Radio emission from neutral hydrogen atoms in the direction of the Orion Nebula, the most nearby regions of high-mass star formation.

Caption

Fig. 1: Radio emission from neutral hydrogen atoms in the direction of the Orion Nebula, the most nearby regions of high-mass star formation.

Credit

Juan D. Soler, University of Vienna, with data from the NRAO's Jansky VLA and NASA's Wide-field Infrared Survey Explorer (WISE).

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