Bahcall–Soneira model of the Milky Way

E938392

The Bahcall–Soneira model of the Milky Way is a pioneering analytic model of our Galaxy’s structure that describes the spatial distribution of stars in its disk and halo, widely used before more detailed modern surveys.

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Statements (45)

Predicate Object
instanceOf Milky Way model
analytic model
galactic structure model
appliesTo Milky Way NERFINISHED
approach phenomenological
semi-empirical
assumes axisymmetric Galaxy
smooth stellar distributions
characterizedBy power-law halo density profile
scale height of the disk
scale length of the disk
coordinateSystem Galactic coordinates
describes spatial distribution of stars in the Milky Way
stellar distribution in the Galactic disk
stellar distribution in the Galactic halo
field astrophysics
galactic astronomy
includesComponent stellar halo
thick disk
thin disk
influenced later Galactic star-count models
inputData observed star counts
stellar luminosity functions
models Galactic disk
Galactic halo
stellar number counts
namedAfter John N. Bahcall NERFINISHED
Raymond J. Soneira NERFINISHED
pioneering yes
predicts distribution of apparent magnitudes of stars
distribution of colors of stars
relatedTo Galactic star-count method
Milky Way structure studies
status historically important
supersededBy modern survey-based Milky Way models
timePeriodOfUse late 20th century
usedFor predicting star counts as a function of Galactic latitude
predicting star counts as a function of Galactic longitude
predicting star counts as a function of magnitude
uses analytic density laws
exponential disk component
spheroidal halo component
wasWidelyUsedBefore Gaia mission NERFINISHED
Sloan Digital Sky Survey NERFINISHED
large digital sky surveys

Referenced by (1)

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

John N. Bahcall notableWork Bahcall–Soneira model of the Milky Way