Backscattering and Line Broadening in Orion
Examination of emission lines in high-velocity-resolution optical spectra of the Orion Nebula confirms that the velocity component on the red wing of the main ionization front emission line is due to backscattering in the Photon Dominated Region. This scattered light component has a weak wavelength...
| Hlavní autoři: | , , |
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| Médium: | Článek |
| Jazyk: | English |
| Vydáno: |
IOP Publishing
2022-01-01
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| Edice: | The Astronomical Journal |
| Témata: | |
| On-line přístup: | https://doi.org/10.3847/1538-3881/ac9f44 |