NGC 7318B is a spiral galaxy

E290089

NGC 7318B is a spiral galaxy in the compact galaxy group Stephan's Quintet, notable for its high-speed collision and interaction with neighboring galaxies.

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All labels observed (1)

Label Occurrences
NGC 7318B is a spiral galaxy canonical 1

Statements (40)

Predicate Object
instanceOf galaxy
spiral galaxy
catalogCode NGC 7318B
discoveredBy Édouard Stephan
hasContext prototype system for studying high-speed galaxy collisions
hasEffectOn large-scale shock front in Stephan's Quintet
hasEnvironment dense group environment
hasGasComponent interstellar medium strongly affected by collision
hasInteractionType galaxy–galaxy collision
ram-pressure interaction with intragroup gas
hasMorphologicalType spiral
hasNotableFeature disturbed spiral structure due to interactions
high-speed collision with other galaxies in Stephan's Quintet
shock fronts in intergalactic medium
strong tidal interactions with neighboring galaxies
hasPhysicalProcess shock heating of gas
star formation triggered by interactions
tidal stripping of gas and stars
hasRole intruder galaxy in Stephan's Quintet collision scenario
interactsWith NGC 7317
NGC 7318B
surface form: NGC 7318A

NGC 7319
NGC 7320
isComponentOf NGC 7318B
surface form: NGC 7318 (pair of galaxies)
isDifferentFrom NGC 7318B
surface form: NGC 7318A
isPartOfSystemWith NGC 7318B
surface form: NGC 7318A
locatedIn constellation Pegasus
memberOf Stephan's Quintet
Stephan's Quintet
surface form: compact galaxy group Stephan's Quintet
observedIn X-ray wavelengths
infrared wavelengths
optical wavelengths
radio wavelengths
partOf Stephan's Quintet
Stephan's Quintet intragroup medium environment
compact galaxy group
redshift non-zero (recessional velocity indicating cosmological distance)
studiedBy Chandra X-ray Observatory
Hubble Space Telescope
Spitzer Space Telescope

Referenced by (1)

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

Stephan's Quintet memberGalaxyType NGC 7318B is a spiral galaxy