GD-1 stream

E502434

The GD-1 stream is a long, thin tidal stream of stars in the Milky Way’s halo, believed to be the remnant of a disrupted globular cluster and a key probe of the Galaxy’s dark matter distribution.

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Statements (42)

Predicate Object
instanceOf astrophysical structure
stellar tidal stream
discoveredBy Carl J. Grillmair NERFINISHED
discoveredIn 2006
discoveredUsing Sloan Digital Sky Survey NERFINISHED
hasAge several billion years
hasComponent old stars
hasDynamics phase-mixed tidal debris
hasKinematics cold stellar stream
hasLength over 60 degrees on the sky
hasMetallicity metal-poor
hasOrbitType highly eccentric orbit
hasPopulation halo stars
hasProgenitorType globular cluster
hasReferenceFrame Galactocentric coordinates
hasShape long thin stream
hasSignificance benchmark system for testing dark matter models
key tracer of Galactic halo structure
hasStellarPopulation old metal-poor stars
hasWidth less than 1 degree on the sky
isCandidateProbeFor dark matter subhalos
isExampleOf cold thin stellar stream
isObservedIn optical wavelengths
isPerturbedBy Galactic bar NERFINISHED
Milky Way disk NERFINISHED
isRemnantOf globular cluster
isSubjectOf dark matter substructure searches
stellar stream dynamical modeling
isUsedToConstrain Milky Way mass distribution
properties of dark matter clumps
locatedIn Milky Way halo NERFINISHED
orbits Milky Way NERFINISHED
originatesFrom disrupted globular cluster
partOf Milky Way galaxy NERFINISHED
showsFeature density variations
gaps
spurs
studiedWith Gaia mission data
Sloan Digital Sky Survey photometry
traces Milky Way halo potential
usedAsProbeFor Milky Way dark matter distribution
Milky Way gravitational potential

Referenced by (1)

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