Perseus molecular cloud complex
E109439
The Perseus molecular cloud complex is a prominent nearby star-forming region rich in cold gas and dust, known for hosting numerous young stellar objects and protostars.
All labels observed (2)
| Label | Occurrences |
|---|---|
| Perseus molecular cloud | 3 |
| Perseus molecular cloud complex canonical | 3 |
Statements (51)
| Predicate | Object |
|---|---|
| instanceOf |
giant molecular cloud
ⓘ
molecular cloud complex ⓘ star-forming region ⓘ |
| contains |
Herbig–Haro objects
ⓘ
surface form:
Herbig-Haro objects
cold molecular gas ⓘ dark clouds ⓘ embedded star clusters ⓘ interstellar dust ⓘ pre-main-sequence stars ⓘ protostars ⓘ reflection nebulae ⓘ young stellar objects ⓘ |
| containsRegion |
Barnard 1
ⓘ
Barnard 5 ⓘ IC 348 ⓘ L1448 ⓘ L1451 ⓘ L1455 ⓘ NGC 1333 ⓘ Perseus OB2 association vicinity ⓘ |
| distanceFromEarth |
approximately 250 to 350 parsecs
ⓘ
approximately 800 to 1150 light-years ⓘ |
| forms |
intermediate-mass stars
ⓘ
low-mass stars ⓘ |
| hasAlternativeName |
Perseus cloud complex
ⓘ
Perseus molecular cloud complex ⓘ
surface form:
Perseus molecular cloud
|
| hasAngularSize | several degrees on the sky ⓘ |
| hasEnvironment | cold ⓘ |
| hasMass | on the order of 10^4 solar masses ⓘ |
| hasNotableFeature |
dense cores
ⓘ
filamentary structure ⓘ outflows from young stars ⓘ |
| hasPhysicalSize | tens of parsecs ⓘ |
| locatedIn |
Gould Belt
ⓘ
Perseus constellation ⓘ |
| observedBy |
Herschel Space Observatory
ⓘ
IRAM 30m telescope ⓘ James Clerk Maxwell Telescope ⓘ
surface form:
JCMT
Planck spacecraft ⓘ
surface form:
Planck satellite
Spitzer Space Telescope ⓘ |
| observedIn |
CO rotational lines
ⓘ
infrared wavelengths ⓘ submillimeter continuum ⓘ |
| partOf | Milky Way ⓘ |
| starFormationActivity | active ⓘ |
| typicalGasTemperature | around 10 Kelvin ⓘ |
| usedForStudyOf |
core mass function
ⓘ
early stages of star formation ⓘ feedback from young stars ⓘ protostellar evolution ⓘ turbulence in molecular clouds ⓘ |
Referenced by (6)
Full triples — surface form annotated when it differs from this entity's canonical label.
this entity surface form:
Perseus molecular cloud
this entity surface form:
Perseus molecular cloud
subject surface form:
NGC 1499
this entity surface form:
Perseus molecular cloud