Measurements of chromospheric densities and geometrical extensions of late-type giant and super-giant stars
Technical Report
·
OSTI ID:6862456
The density sensitivity of the emission lines within the UV 0.01 multiplet of C II near 2325 A was examined in additional late type giants and supergiants with deep LWR high dispersion exposures. The new data support the original contention based on these lines that noncoronal red giants possess geometrically extended chromospheres.
- Research Organization:
- Ohio State Univ., Columbus (USA)
- OSTI ID:
- 6862456
- Report Number(s):
- N-84-17079; NASA-CR-175349
- Country of Publication:
- United States
- Language:
- English
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