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.