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Statements (22)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
gptkb:astrophysical_concept
|
| gptkbp:alsoKnownAs |
gptkb:Eddington_luminosity
|
| gptkbp:appliesTo |
stars
accreting black holes accreting neutron stars |
| gptkbp:c |
speed of light
|
| gptkbp:describes |
maximum luminosity a star can achieve
|
| gptkbp:determines |
balance between radiation pressure and gravitational force
|
| gptkbp:field |
astrophysics
|
| gptkbp:firstDescribed |
1926
|
| gptkbp:form |
L_Edd = (4πGMc)/κ
|
| gptkbp:G |
gravitational constant
|
| gptkbp:hasUnit |
watts
|
| gptkbp:namedAfter |
gptkb:Arthur_Eddington
|
| gptkbp:relatedTo |
affects growth of supermassive black holes
influences stellar evolution limits accretion rates |
| gptkbp:κ |
opacity of the material
|
| gptkbp:מטה |
mass of the object
|
| gptkbp:bfsParent |
gptkb:Arthur_Eddington
|
| gptkbp:bfsLayer |
4
|
| https://www.w3.org/2000/01/rdf-schema#label |
Eddington limit
|