de Vaucouleurs system of galaxy classification

E902178

The de Vaucouleurs system of galaxy classification is an extended and more detailed refinement of the Hubble scheme that categorizes galaxies using a three-dimensional notation incorporating features such as bars, rings, and spiral arm structure.

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Statements (49)

Predicate Object
instanceOf astronomical classification scheme
galaxy morphological classification system
alsoKnownAs de Vaucouleurs revised Hubble system NERFINISHED
de Vaucouleurs revised Hubble–Sandage system NERFINISHED
basedOn Hubble sequence NERFINISHED
capturesFeature inner rings
outer rings
pseudo-rings
classifiesBy bulge-to-disk ratio
degree of arm winding
lens components
presence of bar
ring structures
spiral arm structure
developedBy Gérard de Vaucouleurs NERFINISHED
dimensionIncludes family
stage
variety
distinguishes strongly barred spirals
unbarred spirals
weakly barred spirals
extends Hubble tuning fork diagram NERFINISHED
field extragalactic astronomy
galaxy morphology
goal provide more detailed description of galaxy morphology
includes barred spiral galaxies
elliptical galaxies
irregular galaxies
lenticular galaxies
spiral galaxies
influenced RC2 galaxy catalog classifications
RC3 galaxy catalog classifications NERFINISHED
introducedIn mid-20th century
namedAfter Gérard de Vaucouleurs NERFINISHED
notationExample (r)
(rs)
(s)
SA
SAB
SB
a
b
c
d
e
refines Hubble galaxy classification scheme NERFINISHED
supports continuous sequence of galaxy types
usedIn cataloging nearby galaxies
uses three-dimensional notation

Referenced by (1)

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

Hubble sequence of galaxy classification inspired de Vaucouleurs system of galaxy classification