T Coronae Borealis
E1285706
UNEXPLORED
T Coronae Borealis is a recurrent nova system in the constellation Corona Borealis, known for its rare but dramatic outbursts caused by mass transfer onto a white dwarf from a red giant companion.
All labels observed (1)
| Label | Occurrences |
|---|---|
| T Coronae Borealis canonical | 1 |
How this entity was disambiguated
This entity first appeared as the object of triple T17653994 — resolving that mention is where its identity was fixed. The disambiguator weighed these candidate entities and picked the highlighted one (or “None”, minting a new entity). This is how homonymy is resolved: the same surface form can point to different entities.
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: T Coronae Borealis Context triple: [Corona Borealis, notableVariableStar, T Coronae Borealis]
-
A.
V Coronae Australis
V Coronae Australis is a variable star located in the southern constellation Corona Australis.
-
B.
R Coronae Borealis
R Coronae Borealis is a rare type of hydrogen-deficient, carbon-rich supergiant star famous for its unpredictable, dramatic fades in brightness caused by dust formation.
-
C.
TY Coronae Australis
TY Coronae Australis is a young variable star in the Corona Australis constellation, associated with a nearby star-forming region and circumstellar material.
-
D.
Gamma Coronae Borealis
Gamma Coronae Borealis is a binary star system in the northern constellation Corona Borealis, visible to the naked eye and used as a reference point within the constellation’s distinctive arc.
-
E.
Beta Coronae Borealis
Beta Coronae Borealis is a bright binary star system in the constellation Corona Borealis, known for its chemically peculiar primary component.
- F. None of above. chosen
- G. Unsure - the case is ambiguous/there is not enough information to decide.
NED2
Entity disambiguation (via description)
gpt-5-mini-2025-08-07
Target entity: T Coronae Borealis Target entity description: T Coronae Borealis is a recurrent nova system in the constellation Corona Borealis, known for its rare but dramatic outbursts caused by mass transfer onto a white dwarf from a red giant companion.
-
A.
V Coronae Australis
V Coronae Australis is a variable star located in the southern constellation Corona Australis.
-
B.
R Coronae Borealis
R Coronae Borealis is a rare type of hydrogen-deficient, carbon-rich supergiant star famous for its unpredictable, dramatic fades in brightness caused by dust formation.
-
C.
TY Coronae Australis
TY Coronae Australis is a young variable star in the Corona Australis constellation, associated with a nearby star-forming region and circumstellar material.
-
D.
Gamma Coronae Borealis
Gamma Coronae Borealis is a binary star system in the northern constellation Corona Borealis, visible to the naked eye and used as a reference point within the constellation’s distinctive arc.
-
E.
Beta Coronae Borealis
Beta Coronae Borealis is a bright binary star system in the constellation Corona Borealis, known for its chemically peculiar primary component.
- F. None of above. chosen
Referenced by (1)
Full triples — surface form annotated when it differs from this entity's canonical label.