Leading Arm

E487062

The Leading Arm is a stream of gas extending ahead of the Magellanic Clouds as they orbit the Milky Way, thought to be stripped from these dwarf galaxies by gravitational and hydrodynamic interactions.

All labels observed (2)

Label Occurrences
Leading Arm canonical 1
Leading Arm III 1

How this entity was disambiguated

Statements (50)

Predicate Object
instanceOf astrophysical gas structure ⓘ
gaseous tidal feature ⓘ
high‑velocity cloud complex ⓘ
angularExtent over 60 degrees on the sky ⓘ
associatedWith Large Magellanic Cloud ⓘ
Small Magellanic Cloud ⓘ
composedOf ionized gas ⓘ
neutral hydrogen gas ⓘ
contains cold neutral medium clumps ⓘ
warm ionized gas ⓘ
contrastsWith Magellanic Stream ⓘ
contributesTo gas accretion onto Milky Way ⓘ
discoveredBy radio observations of H I ⓘ
distanceEstimate approximately 20–60 kiloparsecs ⓘ
extendsAheadOf Magellanic Clouds ⓘ
extendsOver tens of kiloparsecs ⓘ
gasPhase multi‑phase medium ⓘ
hasKinematics distinct from Galactic disk rotation ⓘ
negative Galactic‑standard‑of‑rest velocities in some regions ⓘ
hasPhysicalProcessOrigin gravitational interactions with Milky Way ⓘ
hydrodynamic interactions with Milky Way halo gas ⓘ
ram‑pressure stripping ⓘ
tidal stripping ⓘ
hasSubstructure Leading Arm I ⓘ
Leading Arm II ⓘ
Leading Arm III ⓘ
linked to: Leading Arm

Leading Arm IV ⓘ
interactsWith Milky Way circumgalactic medium ⓘ
Milky Way disk gas ⓘ
kinematicallyRelatedTo Magellanic Stream ⓘ
locatedIn Milky Way halo ⓘ
metallicity similar to Magellanic Clouds ⓘ
sub‑solar metallicity ⓘ
modeledBy N‑body simulations of Magellanic System ⓘ
hydrodynamical simulations of Milky Way–Magellanic interaction ⓘ
observationalChallenge confusion with Galactic H I emission ⓘ
observedAs high‑velocity H I emission ⓘ
observedWith Arecibo Observatory ⓘ
Green Bank Telescope ⓘ
Hubble Space Telescope ultraviolet spectroscopy ⓘ
Parkes radio telescope ⓘ
orbitsWith Magellanic Clouds ⓘ
originatesFrom gas stripped from Magellanic Clouds ⓘ
partOf Magellanic System ⓘ
relevance tests models of Milky Way mass and halo structure ⓘ
studiedInContextOf circumgalactic medium ⓘ
galaxy interaction dynamics ⓘ
gas accretion onto galaxies ⓘ
tracedBy 21‑cm line of neutral hydrogen ⓘ
velocityFrame Local Standard of Rest ⓘ

How these facts were elicited

Referenced by (2)

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

Magellanic Stream → containsFeature → Leading Arm ⓘ
Leading Arm → hasSubstructure → Leading Arm III ⓘ
linked to: Leading Arm