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The Shocked Molecular Gas in the Orion Bright Bar
Published online by Cambridge University Press: 04 August 2017
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The Orion bright bar, a bar shaped optical feature, is seen about 2 arcmin southeast of the Trapezium stars in the Orion nebula. Since the bright bar is probably an ionization front seen edge on, this region has an ideal configuration to investigate a shocked region generated by an expanding H II region.
- Type
- I. Star Forming Processes in the Solar Neighborhood
- Information
- Symposium - International Astronomical Union , Volume 115: Star Forming Regions , 1987 , pp. 150 - 153
- Copyright
- Copyright © Reidel 1987
References
Hayashi, M., Hasegawa, T., Gatley, I., and Kaifu, N.: 1985, Monthly Notices Roy. Astron. Soc.
215, 31p.CrossRefGoogle Scholar
Omodaka, T., Hayashi, M., and Hasegawa, T.: 1984, Astrophys. J. (Letters)
282, L77.CrossRefGoogle Scholar
Schloerb, F.P., and Loren, R.B.: 1982, in Symposium on the Orion Nebula to Honor Henry Draper, ed. Glassgold, A.E., Huggins, P.J., and Schucking, E.L. (New York: New York Academy of Science), p32.Google Scholar
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