- Faber-Jackson relation
The Faber-Jackson relation is an early
empirical power-law relation between theluminosity and the central stellarvelocity dispersion of elliptical galaxies, first noted by the astronomersSandra M. Faber and Robert Earl Jackson in1976 . A revision to the relation was published in1991 by astronomer Donald H. Gudehus. The original relation can be expressed mathematically as::
where the index is observed to be very close to 4, as expected from theoretical considerations (see below). The Faber-Jackson relation is an aspect of the fundamental plane of elliptical galaxies and is equivalent to the
Tully-Fisher relation in spiral galaxies. One of its main uses is as a tool for determining distances to external galaxies.Theory
The gravitational potential of a mass distribution of radius and mass is given by the expression:
:
The kinetic energy is (recall is the 1 dimensional velocity dispersion. Therefore 2 = 3V2):
:
:
From the
Virial Theorem ( ) it follows:.
If we assume that the mass to light ratio, , is constant, e.g. we can use this and the above expression to obtain a relation between and :
:.
Let us introduce the surface brightness, and assume this is a constant to get
:.
Using this and combining it with the relation between and , this results in
:
and by rewriting the above expression, we finally obtain the relation between luminosity and velocity dispersion:
:,
that is
:.
When account is taken of the fact that massive galaxies originate from homologous merging, and the fainter ones from dissipation, the assumption of constant surface brightness can no longer be supported. Empirically, surface brightness exhibits a peak at about . The revised relation then becomes
:
for the less massive galaxies, and
:
for the more massive ones. With these revised formulae, the fundamental plane splits into two planes inclined by about 11 degrees to each other.
Even first-ranked cluster galaxies do not have constant surface brightness. A claim supporting constant surface brightness was presented by astronomer
Allan R. Sandage in 1972 based on three logical arguments and his own empirical data. In 1975, Donald Gudehus showed that each of the logical arguments was incorrect and that first-ranked cluster galaxies exhibited a standard deviation of about half a magnitude.Estimating distances to galaxies
Like the Tully-Fisher relation, the Faber-Jackson relation provides a means of estimating the distance to a galaxy, which is otherwise hard to obtain, by relating it to more easily observable properties of the galaxy. In the case of elliptical galaxies, if one can measure the central stellar velocity dispersion, which can be done relatively easily by using
spectroscopy to measure theDoppler shift of light emitted by the stars, then one can obtain an estimate of the true luminosity of the galaxy via the Faber-Jackson relation. This can be compared to theapparent magnitude of the galaxy, which provides an estimate of thedistance modulus and, hence, the distance to the galaxy. By combining a galaxy's central velocity dispersion with measurements of its central surface brightness and radius parameter, it is possible to improve the estimate of the galaxy's distance even more. This standard yardstick, or "reduced galaxian radius-parameter", , devised by Gudehus in 1991, can yield distances, free of systematic bias, accurate to about 31%.External links
* [http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=1976ApJ...204..668F&db_key=AST&data_type=HTML&format=&high=4481ca366126254 The original paper by Faber & Jackson]
* [http://adsabs.harvard.edu/abs/1991ApJ...382....1G Gudehus's revision of the Faber-Jackson relation]ee also
*
Fundamental plane (elliptical galaxies)
*Tully-Fisher relation
*M-sigma relation
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