Hyperfine splitting of [Al VI] 3.66 mu m and the Al isotopic ratio in NGC 6302
The core of planetary nebula NGC 6302 is filled with high-excitation photoionized gas at low expansion velocities. It represents a unique astrophysical situation in which to search for hyperfine structure (HFS) in coronal emission lines from highly ionized species. HFS is otherwise blended by therma...
المؤلفون الرئيسيون: | Casassus, S, Storey, P, Barlow, M, Roche, P |
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التنسيق: | Journal article |
اللغة: | English |
منشور في: |
2005
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مواد مشابهة
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Hyperfine splitting of [Al VI] 3.66 μm and the Al isotopic ratio
حسب: Casassus, S, وآخرون
منشور في: (2005) -
Optical-IR echelle spectroscopy of NGC 6302
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منشور في: (2002) -
The coronal line regions of planetary nebulae NGC 6302 and 6537: 3-13 mu m grating and echelle spectroscopy
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منشور في: (2023-01-01) -
Distribution and Kinematics of H i through Raman He ii Spectroscopy of NGC 6302
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