Triple
T93522
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | Subrahmanyan Chandrasekhar |
E1879
|
entity |
| Predicate | knownFor |
P22
|
FINISHED |
| Object |
Chandrasekhar limit
The Chandrasekhar limit is the maximum mass a white dwarf star can have before collapsing under its own gravity, playing a crucial role in determining its ultimate fate as a neutron star or black hole.
|
E9076
|
NE FINISHED |
Provenance (5 batches)
| Stage | Batch ID | Job type | Status |
|---|---|---|---|
| creating | batch_69a24d1a97dc819094e6c021fe9b05a7 |
elicitation | completed |
| NER | batch_69a24fd28e988190bde699647ee5b16b |
ner | completed |
| NED1 | batch_69a266ebb994819085fb84dd1d2d25ad |
ned_source_triple | completed |
| NED2 | batch_69a2685dc64c8190bd611985d1bc27a3 |
ned_description | completed |
| NEDg | batch_69a267b740388190a321023aa52a539a |
nedg | completed |
Created at: Feb. 28, 2026, 2:07 a.m.