W3(OH)

E476473

W3(OH) is a compact, massive star-forming region and strong OH maser source within the W3 molecular cloud complex, notable for its intense radio and infrared emission.

All labels observed (1)

Label Occurrences
W3(OH) canonical 3

How this entity was disambiguated

Statements (46)

Predicate Object
instanceOf H II region
OH maser source
infrared source
radio source
star-forming region
associatedWith dense molecular gas
dusty core
ultracompact H II region
belongsTo Milky Way galaxy
linked to: Milky Way
distanceFromEarth about 2 kiloparsecs
about 6,000 light-years
emits strong infrared radiation
strong radio continuum emission
has hot molecular core nearby
hasAngularSize sub-arcsecond (for compact core)
hasEnvironment high extinction
high gas density
hasMaserEmission CH3OH
H2O
OH
hasOutflows molecular outflows
hasParallaxMeasurements yes
hasPhysicalProcess gravitational collapse of molecular gas
ionization by massive young stars
maser amplification by population inversion
hasProperMotionMeasurements yes
hasSpectralLineEmission hydroxyl (OH)
methanol (CH3OH)
water (H2O)
hasStarFormation embedded protostars
massive stars
is compact
massive
well-studied maser source
locatedIn Perseus Arm of the Milky Way
linked to: Perseus Spiral Arm

W3 molecular cloud complex
constellation Cassiopeia
linked to: Cassiopeia
near W3 Main
W3(H2O)
observedBy Very Large Array
Very Long Baseline Interferometry
radio interferometers
partOf W3 star-forming complex
usedFor Galactic structure measurements
studies of maser kinematics
studies of massive star formation

How these facts were elicited

Referenced by (3)

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

W3 Main near W3(OH)
W3 hasSubregion W3(OH)