W5 H II region

E478308

W5 H II region is a large ionized hydrogen cloud in the Milky Way notable for active star formation and complex nebular structures.

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Observed surface forms (1)

Surface form Occurrences
Westerhout 5 1

Statements (48)

Predicate Object
instanceOf H II region
emission nebula
interstellar cloud
star-forming region
belongsTo Galactic disk
composedPrimarilyOf ionized hydrogen
contains embedded star clusters
infrared sources
massive OB stars
molecular clouds
protostars
young stellar objects
hasAlternativeName IC 1848 nebular complex NERFINISHED
W5
hasEnvironment dense interstellar medium
hasIonizingSources early B-type stars
massive O-type stars
hasNebularComponent dust
ionized gas
molecular gas
hasPhysicalProcess massive star formation
photoionization
stellar feedback
triggered star formation
hasProcess gas compression at ionization fronts
gas ionization by ultraviolet radiation
hasRoleIn feedback-regulated cloud evolution
galactic star formation
hasStructure bright rims
cavities
dark globules
filaments
pillars
isAssociatedWith IC 1848 star cluster NERFINISHED
isCharacterizedBy active star formation
complex nebular morphology
dust lanes
strong H-alpha emission
isObservedIn infrared wavelengths
optical wavelengths
radio wavelengths
isStudiedFor early stages of stellar evolution
massive star feedback effects
triggered star formation mechanisms
isTypeOf giant H II region
locatedIn Milky Way
Perseus Arm NERFINISHED
partOf Cassiopeia constellation NERFINISHED

Referenced by (2)

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

W3 star-forming region associatedWith W5 H II region
W5 star-forming region alsoKnownAs W5 H II region
this entity surface form: Westerhout 5