Virgo Overdensity

E502432

The Virgo Overdensity is a large, diffuse concentration of stars in the Milky Way’s outer regions, thought to be the remnant of a disrupted dwarf galaxy or stellar stream.

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Statements (43)

Predicate Object
instanceOf Galactic halo substructure
stellar overdensity
stellar stream candidate
angularSize over 1000 square degrees
appearsInConstellation Virgo NERFINISHED
characterizedBy diffuse stellar distribution
large spatial extent
low surface brightness
composedMostlyOf metal-poor stars
old stars
discoveredUsing Sloan Digital Sky Survey NERFINISHED
distanceFromGalacticCenter approximately 6–20 kiloparsecs above or below the Galactic plane
distanceFromSun approximately 6–20 kiloparsecs
evidenceFor ongoing assembly of the Milky Way halo
extendsIntoConstellation Boötes NERFINISHED
Coma Berenices NERFINISHED
Leo NERFINISHED
hasAlternativeName VOD NERFINISHED
Virgo Stellar Overdensity NERFINISHED
hasKinematics distinct from typical Galactic disk stars
suggestive of accreted origin
hasUncertain exact three-dimensional shape
precise progenitor system
total stellar mass
identifiedBy overdensity of F-type main-sequence turnoff stars
overdensity of RR Lyrae stars
locatedIn Galactic halo NERFINISHED
Milky Way
outer regions of the Milky Way
namedAfter Virgo constellation NERFINISHED
observedIn optical wavelengths
relatedTo Monoceros Ring NERFINISHED
Sagittarius Stream NERFINISHED
other Milky Way halo substructures
significanceInAstrophysics constrains models of the Galactic potential
tests hierarchical galaxy formation scenarios
traces past accretion events onto the Milky Way
stellarPopulationType halo stars
studiedUsing photometric surveys
spectroscopic follow-up observations
thoughtToBe evidence of hierarchical galaxy formation
remnant of a disrupted dwarf galaxy
remnant of a stellar stream

Referenced by (1)

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

Milky Way stellar halo hasSubstructure Virgo Overdensity