Perseus cloud complex

E476470

The Perseus cloud complex is a nearby giant molecular cloud in the constellation Perseus that serves as an active region of low- to intermediate-mass star formation.

All labels observed (1)

Label Occurrences
Perseus cloud complex canonical 1

How this entity was disambiguated

Statements (45)

Predicate Object
instanceOf giant molecular cloud
star-forming region
contains Barnard 1
Barnard 5
Herbig–Haro objects
IC 348
L1448
L1455
L1468
NGC 1333
Perseus OB2 association (surrounding region)
dense molecular cores
filamentary molecular structures
molecular outflows
pre-main-sequence stars
protostellar objects
distanceFromEarth approximately 250–350 parsecs
approximately 800–1100 light-years
hasAlternativeName Perseus molecular cloud complex
hasAngularSize several degrees on the sky
hasApproximateMass on the order of 10^4 solar masses
hasEnvironment diffuse molecular gas
embedded young stellar clusters
hasGasComponent molecular hydrogen
hasGasTracer carbon monoxide (CO)
hasRole nearby laboratory for studying low-mass star formation
testbed for theories of clustered star formation
hasStarFormationType intermediate-mass star formation
low-mass star formation
hasSubregion eastern IC 348 region
western NGC 1333 region
is active star-forming region
locatedIn Perseus Arm
locatedInConstellation Perseus
observedIn CO molecular line emission
infrared wavelengths
submillimeter continuum
partOf Milky Way
studiedInContextOf Gould Belt clouds
linked to: Gould Belt

nearby star-forming molecular clouds
surveyedBy 2MASS survey
Herschel Space Observatory
JCMT Gould Belt Survey
Planck satellite
linked to: Planck spacecraft

Spitzer Space Telescope

How these facts were elicited

Referenced by (1)

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