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Deciphering the 3-D Orion Nebula-I: Expanding Shells in the Huygens Region

Based on imaging and spectroscopic data, we develop a 3-D model for the Huygens Region of the Orion Nebula. Theta1OriC , the hottest star in the Trapezium, is surrounded by a wind-blown Central Bubble that opens SW into the Extended Orion Nebula. Outside of this feature lies a layer of ionized gas at about 0.4 pc from Theta1OriC. Both of these features are moving rapidly away from Theta1OriC with an expansion age for the Central Bubble of only 15,000 yrs.

preprint2020arXivOpen access
C. R. O'DellN. P. AbelG. J. Ferland
astro-ph.GA
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Open access3 authors1 topic
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C. R. O'DellN. P. AbelG. J. Ferland

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