Outer Arm

E109438

The Outer Arm is one of the Milky Way galaxy’s major spiral arms, located farther from the galactic center than the Perseus Arm and containing stars, gas, and dust in the outer disk.

All labels observed (1)

Label Occurrences
Outer Arm canonical 1

How this entity was disambiguated

Statements (42)

Predicate Object
instanceOf spiral arm
structure in the Milky Way
belongsTo Galactic spiral pattern
composedOf gas and dust lanes
stellar populations
contains interstellar dust
interstellar gas
stars
distanceFromSun greater than distance of Perseus Arm from Sun
extendsThrough outer Galactic quadrants
fartherFrom Galactic Center than the Perseus Arm
hasAlternativeName Norma–Cygnus Arm
surface form: Norma–Cygnus Arm (in some models)

Outer Galactic Arm
hasPart H II regions
molecular clouds
neutral hydrogen clouds
star-forming regions
hasProperty associated with ongoing star formation
contains relatively low metallicity stars compared to inner arms
contains young stellar objects
isBeyond Perseus Arm
isLessProminentThan Perseus Arm
isLocatedAt larger Galactocentric radius than the Sun
isMajorArmOf Milky Way
isMappedUsing infrared star counts
parallax measurements of masers
surveys of neutral hydrogen
isMoreDistantThan Perseus Arm
isPartOf outer spiral structure of the Milky Way
isTracedBy 21-cm hydrogen line emission
CO molecular line emission
radio observations
locatedIn outer region of the Milky Way galaxy
observedIn infrared wavelengths
radio wavelengths
orientation roughly follows the Milky Way’s global spiral pattern
partOf Milky Way
Galactic thin disk
surface form: Milky Way disk
roleInGalaxy contributes to overall mass distribution of the Milky Way disk
hosts part of the Milky Way’s star formation in the outer disk
studiedBy Galactic structure researchers
radio astronomers

How these facts were elicited

Referenced by (1)

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

Perseus Arm liesInside Outer Arm