W5 H II region
E478308
W5 H II region is a large ionized hydrogen cloud in the Milky Way notable for active star formation and complex nebular structures.
Observed surface forms (1)
| Surface form | Occurrences |
|---|---|
| Westerhout 5 | 1 |
Statements (48)
| Predicate | Object |
|---|---|
| instanceOf |
H II region
ⓘ
emission nebula ⓘ interstellar cloud ⓘ star-forming region ⓘ |
| belongsTo | Galactic disk ⓘ |
| composedPrimarilyOf | ionized hydrogen ⓘ |
| contains |
embedded star clusters
ⓘ
infrared sources ⓘ massive OB stars ⓘ molecular clouds ⓘ protostars ⓘ young stellar objects ⓘ |
| hasAlternativeName |
IC 1848 nebular complex
NERFINISHED
ⓘ
W5 ⓘ |
| hasEnvironment | dense interstellar medium ⓘ |
| hasIonizingSources |
early B-type stars
ⓘ
massive O-type stars ⓘ |
| hasNebularComponent |
dust
ⓘ
ionized gas ⓘ molecular gas ⓘ |
| hasPhysicalProcess |
massive star formation
ⓘ
photoionization ⓘ stellar feedback ⓘ triggered star formation ⓘ |
| hasProcess |
gas compression at ionization fronts
ⓘ
gas ionization by ultraviolet radiation ⓘ |
| hasRoleIn |
feedback-regulated cloud evolution
ⓘ
galactic star formation ⓘ |
| hasStructure |
bright rims
ⓘ
cavities ⓘ dark globules ⓘ filaments ⓘ pillars ⓘ |
| isAssociatedWith | IC 1848 star cluster NERFINISHED ⓘ |
| isCharacterizedBy |
active star formation
ⓘ
complex nebular morphology ⓘ dust lanes ⓘ strong H-alpha emission ⓘ |
| isObservedIn |
infrared wavelengths
ⓘ
optical wavelengths ⓘ radio wavelengths ⓘ |
| isStudiedFor |
early stages of stellar evolution
ⓘ
massive star feedback effects ⓘ triggered star formation mechanisms ⓘ |
| isTypeOf | giant H II region ⓘ |
| locatedIn |
Milky Way
ⓘ
Perseus Arm NERFINISHED ⓘ |
| partOf | Cassiopeia constellation NERFINISHED ⓘ |
Referenced by (2)
Full triples — surface form annotated when it differs from this entity's canonical label.
this entity surface form:
Westerhout 5