Harvard spectral classification of stars
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The Harvard spectral classification of stars is an early 20th-century system that categorizes stars by their spectral characteristics and surface temperatures into types O, B, A, F, G, K, and M, forming the basis of modern stellar classification.
Referenced by (3)
| Subject (surface form when different) | Predicate |
|---|---|
|
Edward Charles Pickering
→
Edward Charles Pickering ("Pickering–Fleming system of stellar classification") → |
notableWork |
|
Hertzsprung–Russell diagram
("Morgan–Keenan classification")
→
|
relatedTo |