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Beta Cephei variables, also known as Beta Canis Majoris stars, are variable stars that exhibit small rapid variations in their brightness due to pulsations of the stars' surfaces, thought due to the unusual properties of iron at temperatures of 200,000 K in their interiors. These stars are usually hot blue-white stars of spectral class B and should not…
History, History of observations & Properties
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stars beta cephei variables variable brightness known pulsations iron class variation star first also canis majoris properties number periods hours
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Beta Cephei variable | related to history | American | 0.60 | section |
| Beta Cephei variable | related to history | Edwin Brant Frost | 0.60 | section |
| Beta Cephei variable | related to history | Beta Cephei | 0.60 | section |
| Beta Cephei variable | related to history | Paul Guthnick | 0.60 | section |
| Beta Cephei variable | related to history | Beta Canis Majoris | 0.60 | section |
| Beta Cephei variable | related to history | Sigma Scorpii | 0.60 | section |
| Beta Cephei variable | related to history | Vesto Slipher | 0.60 | section |
| Beta Cephei variable | related to history | Sigma Scorpii's | 0.60 | section |
| Beta Cephei variable | related to history | Levee | 0.60 | section |
| Beta Cephei variable | related to history | Otto Struve | 0.60 | section |
| Beta Cephei variable | related to history | These | 0.60 | section |
| Beta Cephei variable | related to history | However | 0.60 | section |
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