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

C. R. O'Dell, N. P. Abel, G. J. Ferland

Research output: Contribution to journalArticlepeer-review

15 Scopus citations

Abstract

Based on imaging and spectroscopic data, we develop a 3D model for the Huygens Region of the Orion Nebula. θ1 Ori C, 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 θ1 Ori C. Both of these features are moving rapidly away from θ1 Ori C with an expansion age for the Central Bubble of only 15,000 yr.

Original languageEnglish
Article number46
JournalAstrophysical Journal
Volume891
Issue number1
DOIs
StatePublished - Mar 1 2020

Bibliographical note

Publisher Copyright:
© 2020. The American Astronomical Society. All rights reserved..

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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