Physical conditions of the coronal line region in Seyfert 2 galaxies
Recent studies indicate that the region of emission of coronal lines observed in some active galactic nuclei is located in the internal face of the obscurant toroid; however, there are numerous examples of Seyfert 2 galaxies with significant coronal emission. To clarify this anomaly, here we give so...
| Main Authors: | , |
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| Format: | Article |
| Language: | English |
| Published: |
Colombian Academy of Exact, Physical and Natural Sciences
2021
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| Subjects: | |
| Online Access: | View Fulltext in Publisher |