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Mira variables (/ˈmaɪrə/; named for the prototype star Mira) are a class of pulsating stars characterized by very red colours, pulsation periods longer than 100 days, and amplitudes greater than one magnitude in infrared and 2.5 magnitude at visual wavelengths. They are red giants in the very late stages of stellar evolution, on the asymptotic giant…
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mira variables star stars agb helium period due change changes luminosity dredge-ups pulsating fusion mass carbon-rich carbon variable hydrogen red
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| R Leporis arise from a narrow set of conditions that override the normal tendency for AGB stars to maintain a surplus of oxygen over carbon at their surfaces due to dredge-ups | instance of | Carbon-rich stars | 0.80 | text |
| Mira variables undergo fusion in alternating hydrogen | instance of | Pulsating AGB stars | 0.80 | text |
| helium shells | instance of | Pulsating AGB stars | 0.80 | text |
| which produces periodic deep convection known as dredge-ups | instance of | Pulsating AGB stars | 0.80 | text |
| Mira variable | related to External links | OGLE Atlas | 0.60 | section |
| Mira variable | related to External links | Variable Star Light Curves | 0.60 | section |
| Mira variable | related to External links | Mira Variables | 0.60 | section |
| Mira variable | related to List | The | 0.60 | section |
| Mira variable | related to List | Mira | 0.60 | section |
| Mira variable | related to List | Unless | 0.60 | section |
| Mira variable | related to List | V-band | 0.60 | section |
| Mira variable | related to List | Gaia DR2 | 0.60 | section |
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