Milky Way bulge and bar

E929784

The Milky Way bulge and bar is the dense, elongated central stellar structure of our Galaxy, composed of an old, metal-rich stellar population that dominates its inner gravitational potential and strongly influences its overall dynamics.

All labels observed (3)

How this entity was disambiguated

Statements (51)

Predicate Object
instanceOf galactic bulge
stellar bar
affects orbits of stars in the inner disk
star formation in the inner Galaxy
alignedApproximatelyWith Galactic plane
linked to: Galactic disk
classifiedAs pseudobulge by many studies
composedOf metal-rich stars
old stars
contains RR Lyrae stars
dust
globular clusters
interstellar gas
red clump stars
red giant stars
dominates inner gravitational potential of the Milky Way
drives secular evolution of the Milky Way disk
extendsFrom Galactic center
linked to: Milky Way center
formedPrimarilyBy secular evolution of the Galactic disk
funnels gas toward the Galactic center
hasAge mostly older than 8–10 billion years
hasBarMass of order 10^10 solar masses
hasBulgeMass of order 10^10 solar masses
hasComponent Milky Way bar
Milky Way bulge
linked to: Milky Way center
hasKinematics cylindrical rotation
high velocity dispersion
hasLength about 3–5 kiloparsecs
hasMetallicity near-solar or super-solar for dominant population
hasMetallicityGradient negative with increasing distance from Galactic plane
hasMorphology barred bulge
boxy/peanut-shaped bulge
hasOrientationAngle about 20–30 degrees to the Sun–Galactic-center line
hasResonance corotation resonance in the inner disk
inner Lindblad resonance
hasShape elongated
hasStellarPopulation predominantly metal-rich stellar population
predominantly old stellar population
hasTotalMass several 10^10 solar masses
influences global dynamics of the Milky Way
is non-axisymmetric structure
locatedIn central region of the Milky Way
mayContain small classical bulge component
observedBy COBE satellite
Gaia mission
linked to: Gaia observatory

Spitzer Space Telescope
observedIn infrared wavelengths
partOf Milky Way
patternSpeed of order 30–60 km/s/kpc
supports boxy/peanut bulge via bar instabilities
tracedBy near-infrared star counts
red clump giant stars

How these facts were elicited

Referenced by (3)

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

Schwarzschild method in galactic dynamics appliedTo Milky Way bulge and bar
GD-1 stream isPerturbedBy Galactic bar
linked to: Milky Way bulge and bar
NGC 6603 partOf Milky Way inner regions
subject linked to: open cluster NGC 6603
linked to: Milky Way bulge and bar