Table 5
Spearman correlation coefficients ρ of the relations between the Balmer decrement and the underlying Hβ absorption and the physical parameters for all galaxies (Figs. 14 and 18).
| Variable | log Mstar | μe(H) | log b | 12 + log(O/H) | log SFR |
| Units | M ⊙ | AB mag arcsec-2 | M⊙ yr-1 | ||
|
|
|||||
| All galaxies | |||||
|
|
|||||
| C(Hβ) | 0.39 | –0.38 | –0.16 | 0.49 | 0.33 |
| EW Hβabs | –0.16 | 0.08 | 0.04 | –0.31 | –0.07 |
|
|
|||||
| Excluding AGN | |||||
|
|
|||||
| C(Hβ) | 0.35 | –0.36 | –0.22 | 0.50 | 0.25 |
Notes. Determined using both HI-normal and HI-deficient galaxies.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.