"limit" in inglés with examples - Collocation dictionary inglés
- They are assumed to be near or over the Eddington limit.
- Very large high metallicity stars are probably unstable due to the Eddington limit, and would tend to shed mass during the formation process.
- They are assumed to approach (or potentially exceed) the Eddington limit, i.e., the outward pressure of their radiation is almost strong enough to counteract gravity.
- Above the Eddington limit, the star would generate so much radiation that parts of its outer layers would be thrown off in massive outbursts.
- These are thought to be the hypergiants, near the Eddington limit and rapidly losing mass.
- The Eddington limit is invoked to explain the observed luminosity of accreting black holes such as quasars.
- If the luminosity exceeds the Eddington limit, then the radiation pressure drives an outflow.
- Note that contrary to the standard misconception, the Eddington limit does not require spherical symmetry.
- Some X-ray binaries and active galaxies are able to maintain luminosities close to the Eddington limit for very long times.
- The Eddington limit is not a strict limit on the luminosity of a stellar object.
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