BD+31 643

E459041

BD+31 643 is a young, massive star system located in the Perseus OB2 stellar association, notable for its role in studies of early stellar evolution and circumstellar material.

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Observed surface forms (2)

Surface form Occurrences
BD+31 643 A 0
BD+31 643 B 0

Statements (46)

Predicate Object
instanceOf B-type main-sequence star
B-type main-sequence star
B-type star
binary star system
stellar system
young stellar object
emitsStronglyIn optical
ultraviolet
hasAge a few million years
hasAssociatedDust yes
hasAssociatedReflectionNebula yes
hasCircumstellarMaterial yes
hasColorIndex blue
hasComponent BD+31 643 A NERFINISHED
BD+31 643 B NERFINISHED
hasDeclination +32° (approximate)
hasDistanceFromEarth about 1000 light-years
about 300 parsecs
hasEffectiveTemperature about 15000 K (order of magnitude)
hasEnvironment OB association
star-forming region
hasGalacticPopulation Population I
hasHighMass yes
hasInfraredExcess yes
hasLuminosityClass V
hasNearbyMolecularCloud yes
hasObservedDiskOrRingStructure yes
hasRightAscension 03h 44m (approximate)
hasSpectralType B-type
hasStellarClassification B5 V
hasStellarWind yes
hasVariability possible or low-level
is massive
young
isCataloguedIn Bonner Durchmusterung NERFINISHED
isImportantFor constraining models of circumstellar disks around massive stars
understanding early evolution of B-type stars
isSubjectOf high-resolution imaging studies
polarimetric studies
spectroscopic studies
isUsedForStudyOf circumstellar material
early stellar evolution
protoplanetary environments
locatedIn Perseus OB2 association NERFINISHED
Perseus constellation NERFINISHED
memberOf Perseus OB2 stellar association NERFINISHED

Referenced by (1)

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