Galactic OB associations

E476479

Galactic OB associations are large, loosely bound groupings of young, massive O- and B-type stars distributed throughout the Milky Way, marking regions of recent and ongoing star formation.

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Statements (52)

Predicate Object
instanceOf stellar association
young stellar population
ageRange a few million years
typically less than 30 million years
composedOf B-type stars
O-type stars
massive stars
young stars
dynamicalEvolution disperse into the Galactic field
dynamicalState not in virial equilibrium
hasEffectOn Galactic chemical evolution
Galactic energy budget
interstellar medium
large-scale ionization of the ISM
hasProperty contain early spectral types
dominated by massive stars
gravitationally unbound or marginally bound
large spatial extent
loosely bound
low stellar density
often associated with H II regions
often associated with interstellar gas and dust
often associated with ionized gas
often associated with molecular clouds
often associated with reflection nebulae
short-lived structures
tracing recent star formation
locatedIn Galactic disk
Milky Way
spiral arms of the Milky Way
observedIn infrared wavelengths
optical wavelengths
radio wavelengths via associated gas
ultraviolet wavelengths
relatedTo H II regions NERFINISHED
giant molecular clouds
ionization fronts
open clusters
spiral arm structure
star-forming complexes
stellar feedback processes
superbubbles
supernova remnants
triggered star formation
traces recent star formation in the Galactic disk
typicalMass 10^3 to 10^5 solar masses
typicalSize tens to hundreds of parsecs
typicalVelocityDispersion a few km/s
usedFor mapping spiral structure of the Milky Way
studying early stellar evolution
studying feedback from massive stars
studying massive star formation

Referenced by (1)

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

Cassiopeia OB associations isPartOf Galactic OB associations