Triangulum–Andromeda overdensity

E539432

The Triangulum–Andromeda overdensity is a large, diffuse stellar structure in the outer regions of the Milky Way, thought to be the remnant of a disrupted dwarf galaxy or tidal stream.

All labels observed (2)

Label Occurrences
TriAnd overdensity 1
Triangulum–Andromeda overdensity canonical 1

How this entity was disambiguated

Statements (40)

Predicate Object
instanceOf Galactic halo substructure
stellar overdensity
stellar structure
tidal debris candidate
belongsTo outer Galactic halo substructures
composedOf metal-poor stars
old stars
discoveredUsing Sloan Digital Sky Survey
extendsAcrossConstellation Andromeda
Pisces
Triangulum
hasAlternativeName TriAnd
TriAnd overdensity
hasAngularExtent tens of degrees on the sky
hasApproximateDistanceFromSun 20–30 kiloparsecs
hasEstimatedAge several billion years
hasKinematics distinct from Galactic disk
halo-like velocities
hasMetallicity low metallicity
hasMorphology large diffuse structure
hasObservationMethod photometric surveys
spectroscopic follow-up
hasScientificInterest traces past accretion events
hasShape irregular
hasStellarPopulation main-sequence turnoff stars
red giant branch stars
hasTypeOfStructure low-surface-brightness feature
hasUncertainOrigin true
identifiedBy star count overdensities
isCandidateRemnantOf disrupted dwarf galaxy
tidal stream
isDifferentFrom Monoceros Ring
Sagittarius tidal stream
linked to: Sagittarius Stream
isEvidenceFor accretion of dwarf galaxies by the Milky Way
hierarchical formation of the Milky Way
isPartOf large-scale substructure in the Milky Way halo
locatedIn Galactic halo
outer regions of the Milky Way
partOf Milky Way
studiedInWavelength optical

How these facts were elicited

Referenced by (2)

Full triples — surface form annotated when it differs from this entity's canonical label.

Monoceros Ring relatedStructure Triangulum–Andromeda overdensity
Triangulum–Andromeda overdensity hasAlternativeName TriAnd overdensity
linked to: Triangulum–Andromeda overdensity