W75N star-forming region

E479071

W75N is a compact, massive star-forming region within the Cygnus X complex, notable for its dense molecular gas, young stellar objects, and intense maser and radio continuum emission.

All labels observed (1)

Label Occurrences
W75N star-forming region canonical 1

How this entity was disambiguated

Statements (46)

Predicate Object
instanceOf H II region ⓘ
massive star-forming region ⓘ
radio source ⓘ
star-forming region ⓘ
associatedWith embedded protostars ⓘ
massive star formation ⓘ
belongsTo Milky Way Galaxy ⓘ
linked to: Milky Way
contains dense molecular gas ⓘ
hydroxyl masers ⓘ
methanol masers ⓘ
ultracompact H II regions ⓘ
water masers ⓘ
young stellar objects ⓘ
distanceEstimate a few kiloparsecs from the Sun ⓘ
environment high extinction ⓘ
high gas density ⓘ
exhibits intense maser emission ⓘ
strong radio continuum emission ⓘ
hasComponent cluster of young stellar objects ⓘ
multiple compact radio sources ⓘ
hasKinematics complex gas motions ⓘ
infall and outflow signatures ⓘ
hasPhysicalProcess feedback from massive young stars ⓘ
gravitational collapse of molecular gas ⓘ
ionization of surrounding gas ⓘ
shock excitation of masers ⓘ
hasProperty compact ⓘ
massive ⓘ
locatedInConstellation Cygnus ⓘ
observedIn infrared wavelengths ⓘ
millimeter wavelengths ⓘ
radio wavelengths ⓘ
submillimeter wavelengths ⓘ
observedWith Very Large Array ⓘ
Very Long Baseline Interferometry ⓘ
infrared space telescopes ⓘ
single-dish radio telescopes ⓘ
partOf Cygnus X complex ⓘ
shows jets from young stellar objects ⓘ
outflows ⓘ
tracedBy CO molecular line emission ⓘ
NH3 emission ⓘ
dust continuum emission ⓘ
usedFor studies of maser variability ⓘ
studies of massive star formation ⓘ
studies of protostellar outflows ⓘ

How these facts were elicited

Referenced by (1)

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

Cygnus X star-forming region → contains → W75N star-forming region ⓘ