NGC 1850

E512284

NGC 1850 is a massive, young star cluster in the Large Magellanic Cloud notable for its unusual structure and intense star-forming activity.

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Statements (46)

Predicate Object
instanceOf star cluster
young massive cluster
age tens of millions of years
ageClass young
catalogCode NGC 1850 NERFINISHED
cataloguedIn New General Catalogue of Nebulae and Clusters of Stars NERFINISHED
contains B-type stars
X-ray sources
massive O-type stars
pre-main-sequence stars
variable stars
discoveredIn 19th century
distanceFromEarth approximately 160000 light-years
approximately 50 kiloparsecs
environment star-forming region of the Large Magellanic Cloud
hasComponent central compact cluster
ionized gas
surrounding stellar association
hasFeature intense star-forming activity
nebular emission in and around the cluster
presence of blue straggler candidates
presence of pre-main-sequence stars
rich population of massive stars
hasResearchInterest early dynamical evolution of star clusters
interaction between massive stars and surrounding gas
testing theories of cluster formation
hasUnusualProperty central compact cluster with surrounding stellar association
contains multiple stellar populations
double-cluster-like structure
ring-like distribution of stars
hostGalaxy Large Magellanic Cloud NERFINISHED
locatedIn Doradus constellation NERFINISHED
Large Magellanic Cloud NERFINISHED
massClass massive
memberOf New General Catalogue NERFINISHED
observedBy Hubble Space Telescope NERFINISHED
ground-based telescopes
observedIn X-ray wavelengths
optical wavelengths
ultraviolet wavelengths
partOf Magellanic Clouds system NERFINISHED
skyPosition southern celestial hemisphere
usedForStudyOf cluster dynamics
massive star formation
multiple stellar populations in clusters
stellar evolution in young clusters

Referenced by (2)

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

Dorado contains NGC 1850
constellation Dorado containsDeepSkyObject NGC 1850
subject surface form: Dorado