The Tully-Fisher relation Eq. (10.1) relates the absolute
luminosity
of a galaxy to its circular velocity. Now suppose we
were able to measure the proportionality constant, by determining the
absolute luminosity for galaxies with known distance. Then
by just measuring the circular velocity of a spiral galaxy, we could
infer its absolute luminosity, and hence from its apparent magnitude
obtain the distance, since
| (10.13) |
Therefore, the Tully-Fisher relation can be used as a standard candle,
since it allows us to determine the absolute luminosity from the
distance independent quantity
.
The fundamental plane relation plotted in Figure 10.4 can also
be used as a standard candle: all we need to do is measure the velocity
dispersion of the stars
from a spectrum, and determine the
surface brightness (recall that the surface brightness
is distance
independent). By putting the E galaxy onto Figure 10.4, we then
find
. And so from the apparent size of the galaxy, we can
estimate its distance.
Both these methods are widely used, since measuring velocities is relatively easy from a good quality spectrum, and can be done even for faint and/or distant galaxies. And since the scatter in the relations is small, we can obtain a relatively accurate distance estimate.