Hubble V

E500405

Hubble V is a massive, bright star-forming nebula in the Triangulum Galaxy, notable as one of the largest known H II regions in the Local Group.

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Statements (47)

Predicate Object
instanceOf H II region
emission nebula
star-forming nebula
belongsToCategory giant extragalactic H II regions
star-forming regions in M33
catalogDesignation Hubble V NERFINISHED
composedOf dust
ionized hydrogen gas
discoveredBy Edwin Hubble NERFINISHED
distanceFromEarth approximately 2.7 million light-years
approximately 840 kiloparsecs
emits nebular emission lines
strong hydrogen recombination lines
environment star-forming disk of M33
hasAstrophysicalProcess gas heating and cooling
photoionization
radiation pressure from massive stars
stellar winds
hasNotableCharacteristic contains embedded star clusters
contains numerous young massive stars
one of the largest known H II regions in the Local Group
site of active massive star formation
hasPhysicalProperty bright
giant H II complex
luminous in H-alpha
massive
hasResearchInterest chemical abundances in the Triangulum Galaxy
initial mass function in giant H II regions
structure of extragalactic H II complexes
hostGalaxy NGC 598 NERFINISHED
hostGalaxyType spiral galaxy
ionizedBy massive O-type stars
young stellar population
locatedIn M33 NERFINISHED
Triangulum Galaxy NERFINISHED
memberOf Local Group NERFINISHED
namedAfter Edwin Hubble NERFINISHED
observedBy Hubble Space Telescope NERFINISHED
ground-based optical telescopes
radio observatories
observedIn infrared wavelengths
optical wavelengths
radio wavelengths
partOf interstellar medium of the Triangulum Galaxy
studiedFor feedback from massive stars
massive star formation in external galaxies
properties of giant H II regions

Referenced by (1)

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

NGC 604 alternativeName Hubble V