W3 star-forming region

E109440

W3 star-forming region is a massive, active stellar nursery in the Milky Way known for its dense molecular clouds and prolific formation of young, high-mass stars.

All labels observed (1)

Label Occurrences
W3 star-forming region canonical 1

How this entity was disambiguated

Statements (49)

Predicate Object
instanceOf H II region
molecular cloud complex
star-forming region
stellar nursery
associatedWith W4 star-forming region
surface form: W4 H II region

W5 H II region
catalogDesignation W3
constellation Cassiopeia
contains W3 Main
W3 North
W3(OH)
dense molecular clouds
embedded star clusters
giant molecular cloud
infrared sources
maser sources
massive star-forming cores
ultracompact H II regions
young stellar objects
discoveredBy radio observations of the Milky Way
distanceFromEarth about 2 kiloparsecs
about 6000 light-years
hasAgeRange less than a few million years
hasEnvironment dense interstellar medium
strong UV radiation fields
hasProperty active
high extinction
massive
rich in molecular gas
hasStarFormationMode spontaneous star formation
triggered star formation
knownFor clustered star formation
high-mass star formation
ongoing star formation
locatedIn Milky Way
Perseus Arm
observedIn X-ray wavelengths
infrared wavelengths
radio wavelengths
submillimeter wavelengths
partOf Galactic plane
W3/W4/W5 complex
studiedFor cluster formation
feedback from massive stars
massive star formation processes
tracedBy CO emission
dust continuum emission
methanol masers
water masers

How these facts were elicited

Referenced by (1)

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

Perseus Arm contains W3 star-forming region