Table 1
Sample properties.
| Property | Mice | IC 1623 | NGC 6090 | NGC 2623 |
|
|
||||
| CALIFA ID | 577 (A); 939 (B) | – | 2945 | 213 |
| RA | 12 46 10.7 | 01 07 46.3 | 16 11 40.8 | 08 38 23.8 |
| Dec | +30 43 38 | –17 30 32 | +52 27 27 | +25 45 17 |
| Interaction stage | IIIa | IIIb | IIIb | IV |
| z | 0.022049 | 0.020067 | 0.029304 | 0.018509 |
| Scale (kpc/′′) | 0.47 | 0.42 | 0.61 | 0.39 |
| HLR (kpc) | 4.6 (A); 3.8 (B) | 2.8 | 4.2 | 3.3 |
| Stellar mass (M⊙) | 1.2 × 1011 (A), 1.5 × 1011 (B) | 3.9 × 1010 | 6.8 × 1010 | 5.4 × 1010 |
| log(LIR[L⊙]) | 10.62 | 11.65 | 11.51 | 11.54 |
| SFR30Myr (M⊙/yr) | 3 (A), 2 (B) | 20 | 51 | 8 |
Notes. Rows from top to bottom are: (1) CALIFA identification number, (2) and (3) right ascension and declination from Equinox J2000 extracted from Sanders et al. (2003), (4) interaction stage according to Veilleux et al. (2002) classification based on the optical morphologies, (5) redshift extracted from NED webpage, (6) spatial scale, (7) half light radius, (8) stellar masses extracted from Wild et al. (2014), Cortijo-Ferrero et al. (2017a,b), (9) infrared luminosities LIR = L(8−1000) μm from IRAS fluxes extracted from Sanders et al. (2003) for the LIRGs. They are in logarithm and in units of solar bolometric luminosity, L⊙ = 3.83 × 1033 erg s-1. Mice LIR is extracted from Wild et al. (2014) and (10) SFR calculated in the last 30 Myr, from the spectral synthesis in this paper.
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.