3 ms·
Its explained on the next page(it a simplification) In fact, by relaxing some of the assumptions made above, we have the more general relationship: L ∝ V 2/(+s
by FrozenVoid 10y ago
Its explained on the next page(it a simplification)
In fact, by relaxing some of the assumptions made above,
we have the more general relationship: L ∝ V
2/(+s+q−t)
opt
(here s, q and t can be band-
dependent) that can be even more complex and non-linear when the scaling laws (2), (3),
(4) are not just power laws. As a matter of fact, in several different large samples of galaxies
it has been found that the TF has different slope and scatter in different bands: a I ≃ 10,
s I ∼ 0.4mag, while a B ≃ 7.7, s B ∼ 0.5mag (Pierce & Tully 1992), (Salucci et al. 1993).
Moreover, a non linearity in the TF is often found at low rotation velocities (Aaronson et
al. 1982).
- nonbel 10y agoThanks, I will take a closer look.