- #71
turbo
Gold Member
- 3,165
- 56
The Tully-Fisher relation can be used as an estimate of distance to spiral galaxies. By observing the velocity dispersion in such a spiral, the mass of the galaxy can be estimated, and using this mass figure, one can compare the observed luminosity of the galaxy with the luminosity expectation value (from the estimated mass) and obtain a distance measure that is independent of redshift. There is a paper on this subject (written by a collaborator on another paper that we submitted recently) that is currently under review, and I will link to a preprint as soon as it is accepted.Jorrie said:My guess is that above the present Cepheid limit of about z ~ 0.1, there is no other known method than the SNe 1a, or is there?