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Tully-Fisher and Fundamental plane relations as standard candles

The Tully-Fisher relation Eq. (10.1) relates the luminosity $ L$ of a galaxy to its circular velocity. Now suppose we were able to measure the proportionality constant, by determining the luminosity for galaxies with known distance. Then by just measuring the circular velocity of a spiral galaxy, we could infer its luminosity hence absolute magnitude $ M$, and consequently from its apparent magnitude $ m$ obtain the distance $ r$, since

$\displaystyle m-M=5\log(r)-5\,.$ (10.13)

Therefore, the Tully-Fisher relation can be used as a standard candle, since it allows us to determine the luminosity from the distance independent quantity $ V_c$. Note also that $ V_c$ is relatively easy to determine from spectra, and so we have found a good way of measuring distances to distant galaxies!

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 $ \sigma $ from a spectrum, and determine the intensity $ I_e$ (recall that the surface brightness and hence also $ I_e$ is distance independent). By putting the E galaxy onto Figure 10.4, we then find $ R_e$. 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.


next up previous contents
Next: Galaxy luminosity function Up: Galaxy statistics Previous: The Faber-Jackson relation in
Tom Theuns
平成19年2月7日