Table 2.
Mean (and median) stellar mass Mstar, SFR, and sSFR for the different LIRG subsamples.
| Sample | # | Mstar | SFR | sSFR |
|---|---|---|---|---|
| (1010 M⊙) | (M⊙ yr−1) | (Gyr−1) | ||
| (1) | (2) | (3) | (4) | (5) |
| All LIRGs | 24 | 5.6 ± 3.2 (4.8) | 29.4 ± 19.9 (26.9) | 0.63 ± 0.58 (0.46) |
| LIRGs w/o AGN | 17 | 4.9 ± 3.1 (4.6) | 29.9 ± 21.4 (27.5) | 0.74 ± 0.66 (0.57) |
| LIRGs w AGN | 7 | 7.4 ± 2.7 (7.8) | 28.0 ± 17.2 (26.3) | 0.35 ± 0.12 (0.32) |
| 0 RD | 8 | 6.6 ± 3.4 (5.5) | 28.0 ± 14.7 (25.0) | 0.47 ± 0.19 (0.50) |
| 0 PD | 7 | 5.7 ± 3.1 (4.3) | 23.6 ± 7.9 (26.3) | 0.55 ± 0.43 (0.35) |
| 1 | 4 | 2.5 ± 1.2 (2.8) | 8.0 ± 3.0 (8.9) | 0.35 ± 0.12 (0.31) |
| 2 | 5 | 6.5 ± 3.1 (7.0) | 56.8 ± 18.3 (52.5) | 1.23 ± 1.00 (0.76) |
Notes. Columns: (1): Sample and subsample: class 0 identifies isolated disks, class 1 denotes interacting systems, and class 2 stands for mergers (see Sect. 2). Subsamples of LIRGs with (w AGN) and without (w/o AGN) AGN are shown. (2): Number of objects in each sample; (3): Stellar mass in units of 1010 M⊙; (4): SFR in units of M⊙ yr−1; (5): Specific SFR (sSFR = SFR/Mstar) in units of Gyr−1.
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.