Chamaeleon molecular clouds
E459018
The Chamaeleon molecular clouds are a nearby complex of dark interstellar clouds rich in gas and dust, known as an active region of low-mass star formation in the southern sky.
All labels observed (1)
| Label | Occurrences |
|---|---|
| Chamaeleon molecular clouds canonical | 1 |
How this entity was disambiguated
This entity first appeared as the object of triple T4617528 — 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.
Target entity: Chamaeleon molecular clouds Context triple: [Gould Belt, contains, Chamaeleon molecular clouds]
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A.
Corona Australis molecular cloud complex
The Corona Australis molecular cloud complex is a nearby star-forming region rich in dense gas and dust, known for hosting young stellar objects and reflection nebulae in the constellation Corona Australis.
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B.
Perseus molecular cloud complex
The Perseus molecular cloud complex is a prominent nearby star-forming region rich in cold gas and dust, known for hosting numerous young stellar objects and protostars.
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C.
Orion Molecular Cloud Complex
The Orion Molecular Cloud Complex is a vast star-forming region in the constellation Orion, rich in gas, dust, and young stellar objects, and one of the most studied nurseries of massive stars in the Milky Way.
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D.
Monoceros OB2 association
Monoceros OB2 association is a large stellar grouping in the constellation Monoceros, notable for its young, massive stars and active star-forming regions such as the Rosette Nebula.
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E.
Physical Processes in the Interstellar Medium
Physical Processes in the Interstellar Medium is a foundational astrophysics textbook that systematically explains the physics governing gas, dust, radiation, and plasma in the space between stars.
- F. None of above. chosen
- G. Unsure - the case is ambiguous/there is not enough information to decide.
Target entity: Chamaeleon molecular clouds Target entity description: The Chamaeleon molecular clouds are a nearby complex of dark interstellar clouds rich in gas and dust, known as an active region of low-mass star formation in the southern sky.
-
A.
Corona Australis molecular cloud complex
The Corona Australis molecular cloud complex is a nearby star-forming region rich in dense gas and dust, known for hosting young stellar objects and reflection nebulae in the constellation Corona Australis.
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B.
Taurus molecular cloud complex (projected association)
The Taurus molecular cloud complex (projected association) is a nearby star-forming region in the constellation Taurus, rich in dark molecular clouds and young stellar objects studied as a key site of low-mass star formation.
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C.
Perseus molecular cloud complex
The Perseus molecular cloud complex is a prominent nearby star-forming region rich in cold gas and dust, known for hosting numerous young stellar objects and protostars.
-
D.
Orion Molecular Cloud Complex
The Orion Molecular Cloud Complex is a vast star-forming region in the constellation Orion, rich in gas, dust, and young stellar objects, and one of the most studied nurseries of massive stars in the Milky Way.
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E.
Monoceros OB2 association
Monoceros OB2 association is a large stellar grouping in the constellation Monoceros, notable for its young, massive stars and active star-forming regions such as the Rosette Nebula.
- F. None of above. chosen
Statements (48)
| Predicate | Object |
|---|---|
| instanceOf |
molecular cloud complex
ⓘ
star-forming region ⓘ |
| ageOfStellarPopulation | a few million years ⓘ |
| catalogCode |
Cha I
NERFINISHED
ⓘ
Cha II ⓘ Cha III NERFINISHED ⓘ |
| contains |
Chamaeleon I molecular cloud
NERFINISHED
ⓘ
Chamaeleon II molecular cloud NERFINISHED ⓘ Chamaeleon III molecular cloud NERFINISHED ⓘ Chamaeleon IV molecular cloud NERFINISHED ⓘ dark nebulae ⓘ reflection nebulae ⓘ |
| containsObjectType |
Herbig–Haro objects
NERFINISHED
ⓘ
dense cores ⓘ pre-main-sequence stars ⓘ protoplanetary disks ⓘ protostars ⓘ |
| containsStellarAssociation |
Chamaeleon I association
NERFINISHED
ⓘ
Chamaeleon II association NERFINISHED ⓘ |
| distanceFromEarth |
approximately 150 parsecs
ⓘ
approximately 500 light-years ⓘ |
| environmentType | nearby dark cloud complex ⓘ |
| gasComponent | molecular hydrogen ⓘ |
| hasAngularSize | several degrees on the sky ⓘ |
| hasExtinction | high visual extinction regions ⓘ |
| hasNotableRegion |
Cha I North
NERFINISHED
ⓘ
Cha I South NERFINISHED ⓘ Cha II core NERFINISHED ⓘ |
| hasStarFormationActivity | ongoing ⓘ |
| hasStarFormationEfficiency | relatively low ⓘ |
| hasStarFormationMode | low-mass dominated ⓘ |
| knownFor |
T Tauri stars
ⓘ
low-mass star formation ⓘ young stellar objects ⓘ |
| locatedInConstellation | Chamaeleon NERFINISHED ⓘ |
| locatedInSkyHemisphere | southern celestial hemisphere ⓘ |
| observedInWavelength |
infrared
ⓘ
millimeter ⓘ optical ⓘ |
| partOf | Milky Way NERFINISHED ⓘ |
| richIn |
interstellar dust
ⓘ
interstellar gas ⓘ |
| surveyedBy |
ESO telescopes
NERFINISHED
ⓘ
Herschel Space Observatory NERFINISHED ⓘ IRAS NERFINISHED ⓘ Spitzer Space Telescope NERFINISHED ⓘ |
| tracedBy | CO emission ⓘ |
| usedAs | laboratory for low-mass star formation studies ⓘ |
How these facts were elicited
The pipeline generated the facts above by prompting gpt-5.1 with this entity's name + description and the instruction below.
You are a knowledge base construction expert. Given a subject entity and a description of it, return factual statements that you know for the subject as a JSON list of dictionaries(triples), where keys must be "subject", "predicate" and "object". The number of facts may be very high, between 25 to 50 or more, for very popular subjects. For less popular subjects, the number of facts can be very low, like 5 or 10. # Requirements - If you don't know the subject at all, return an empty list. - If the subject is not a named entity, return an empty list. - Include at least one triple where predicate is "instanceOf". - Do not get too wordy. - Separate several objects into multiple triples with one object.
Subject: Chamaeleon molecular clouds Description of subject: The Chamaeleon molecular clouds are a nearby complex of dark interstellar clouds rich in gas and dust, known as an active region of low-mass star formation in the southern sky.
Referenced by (1)
Full triples — surface form annotated when it differs from this entity's canonical label.