Leading Arm of the Magellanic System

E481656

The Leading Arm of the Magellanic System is a vast stream of gas pulled from the Magellanic Clouds that extends ahead of their orbit around the Milky Way, helping astronomers study galaxy interactions and gas accretion.

All labels observed (2)

How this entity was disambiguated

Statements (47)

Predicate Object
instanceOf astrophysical structure ⓘ
gaseous stream ⓘ
high‑velocity cloud complex ⓘ
associatedWith Large Magellanic Cloud ⓘ
Small Magellanic Cloud ⓘ
classification component of the Magellanic gaseous debris ⓘ
composedOf ionized gas ⓘ
neutral hydrogen gas ⓘ
contains cold neutral gas ⓘ
multiple gas clumps and filaments ⓘ
warm ionized gas ⓘ
coordinateSystem often described in Magellanic coordinates ⓘ
directionRelativeToMagellanicClouds leading ⓘ
discoveredThrough H I 21‑cm surveys of the Galactic halo ⓘ
environment low‑metallicity halo environment ⓘ
extendsAheadOf orbit of the Magellanic Clouds around the Milky Way ⓘ
extendsOver tens of degrees on the sky ⓘ
frameOfReference Milky Way rest frame ⓘ
gasFlowDirection toward the Milky Way disk ⓘ
gasPhase multi‑phase medium ⓘ
hasKinematics distinct from the Magellanic Stream ⓘ
hasRole source of future star‑forming material for the Milky Way ⓘ
hasUncertain exact origin and formation mechanism ⓘ
helpsConstrain mass distribution of the Milky Way halo ⓘ
orbital history of the Magellanic Clouds ⓘ
helpsTest models of the Magellanic Clouds’ first infall scenario ⓘ
interactsWith Milky Way halo gas ⓘ
isAsymmetricWithRespectTo Magellanic Stream ⓘ
locatedIn Galactic halo of the Milky Way ⓘ
metallicityRelativeToMilkyWayDisk sub‑solar ⓘ
observationalChallenge confusion with other high‑velocity clouds ⓘ
observedIn radio wavelengths ⓘ
ultraviolet absorption lines ⓘ
originatesFrom ram‑pressure stripping by the Milky Way halo gas ⓘ
tidal interactions between the Magellanic Clouds and the Milky Way ⓘ
partOf Magellanic System ⓘ
Magellanic gaseous system ⓘ
relatedPhenomenon gas accretion onto galaxies ⓘ
tidal stripping in galaxy groups ⓘ
relatedTo Magellanic Stream ⓘ
studiedBy radio surveys of the southern sky ⓘ
subjectOf numerical simulations of the Magellanic System ⓘ
tracedBy 21‑cm H I emission ⓘ
usedFor probing the Milky Way circumgalactic medium ⓘ
studying galaxy interactions ⓘ
studying gas accretion onto the Milky Way ⓘ
velocityType high‑velocity gas relative to the Galactic disk ⓘ

How these facts were elicited

Referenced by (2)

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

Magellanic Bridge → relatedTo → Leading Arm of the Magellanic System ⓘ
Magellanic Stream → relatedTo → Leading Arm of Magellanic System ⓘ
linked to: Leading Arm of the Magellanic System