Figure 9.
Distribution of the width (σ) of the spectral lines and the continuum slope for a sample of 28 galaxies with very clear emission lines. As a reference, the continuum level of a mR = 20 galaxy is ∼5 × 10−18 erg cm−2 Å−1.
Distribution of the width (σ) of the spectral lines and the continuum slope for a sample of 28 galaxies with very clear emission lines. As a reference, the continuum level of a mR = 20 galaxy is ∼5 × 10−18 erg cm−2 Å−1.
