NGC 1672

E513037

NGC 1672 is a barred spiral galaxy notable for its prominent central bar, active star-forming regions, and striking dust lanes, located in the southern constellation Dorado.

Jump to: Statements Referenced by

Statements (46)

Predicate Object
instanceOf barred spiral galaxy
apparentMagnitudeV ~10.3
apparentSize ~6.6 × 5.5 arcminutes
catalog New General Catalogue NERFINISHED
constellation Dorado NERFINISHED
contains H II regions
massive young star clusters
declination −59° 15′ (approx)
discoveredBy James Dunlop NERFINISHED
discoveryYear 1826
distanceFromEarth ~18 megaparsecs
~60 million light-years
environment field galaxy or loose group member
galaxyType barred spiral
hasActivity active star formation
hasBar strong bar
hasBulge bright central bulge
hasDust interstellar dust in disk
hasFeature dust lanes
nuclear star-forming ring
prominent central bar
ring-like structure
spiral arms
hasGas molecular gas (H2)
neutral hydrogen (H I)
hasNucleus active galactic nucleus candidate
hasSpiralStructure grand-design spiral
hasStarFormationRegion central ring
spiral arms
HubbleType SBbc
inclination moderately inclined to line of sight
isTargetOf Chandra X-ray Observatory observations
Hubble Space Telescope observations
locatedInRegion southern sky
morphologicalType SB(r)bc
observedIn X-ray wavelengths
infrared wavelengths
optical wavelengths
otherDesignation ESO 118-G023 NERFINISHED
IRAS 04432-5948 NERFINISHED
partOf local universe
radialVelocity ~1320 km/s
redshift ~0.0044
rightAscension 04h 45m (approx)
showsDust prominent dust lanes along bar
spectralFeatures emission lines from H II regions

Referenced by (3)

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

Dorado contains NGC 1672
constellation Dorado containsDeepSkyObject NGC 1672
subject surface form: Dorado
constellation Dorado containsGalaxy NGC 1672
subject surface form: Dorado