Table 4
A summary of the main properties of the Mice galaxies measured in this paper.
| Parameter | NGC 4676A (NW) | NGC 4676B (SE) |
|
|
||
| B/Ta | 0 (SBd) | 0.5 (S0/a) |
| vnucleus,gas (km s-1)b | 6585 | 6581 |
| vnucleus,stars (km s-1)b | 6652 | 6493 |
| M∗ (1011 M⊙)c | 1.2 | 1.5 |
| SFR ( M⊙/yr)d | ~6 | ~2 |
| P/kwind (106 K cm-3)e | 4.8 | ... |
| Ṁout ( M⊙ yr-1)e | 8−20 | ... |
| Morphological PAf | 2.8 | 33.2 |
| Kinematic PAstarsf | 33.9, 27.6 | 165.4, 150.4 |
| Kinematic PAgasf | 31.9, 24.5 | 154.4, 165.0 |
Notes. For a summary of properties available from the literature see Table 1.
Bulge-to-total flux ratio in the I-band, from image decomposition of HST-ACS image (Sect. 4.1).
Recessional velocity, from kinematic fits to the central spaxel with the highest V-band luminosity (Sect. 4).
Total stellar mass, from full spectrum decomposition assuming a Salpeter IMF (Sect. 5).
Total SFR taken from the median of CALIFA and multiwavelength measurements (Sect. 7).
The ram pressure and mass outflow rate of the bi-conical wind from NGC 4676A (Sect. 8).
Position angles (approaching and receding for kinematic PAs), measured within 10′′ (Barrera-Ballesteros et al., in prep., Sect. 4).
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