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A stellar wind is a flow of gas ejected from the upper atmosphere of a star. It is distinguished from the bipolar outflows characteristic of young stars by being less collimated, although stellar winds are not generally spherically symmetric.
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stars winds stellar wind mass massive solar driven star types sun corona upper atmosphere young ends lives often 10 displaystyle
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Stellar wind | is a | flow of gas ejected from the upper atmosphere of a star | 0.90 | text |
| carbon | instance of | Such winds are driven by radiation pressure on the resonance absorption lines of heavy elements | 0.80 | text |
| nitrogen | instance of | Such winds are driven by radiation pressure on the resonance absorption lines of heavy elements | 0.80 | text |
| the Sun | instance of | that are able to escape the star's gravity because of the high temperature of the corona.Stellar winds from main-sequence stars do not strongly influence the evolution of lower-… | 0.80 | text |
| O stars | instance of | for more massive stars | 0.80 | text |
| the mass loss can result in a star shedding as much as 50 | instance of | for more massive stars | 0.80 | text |
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