Table 1.
Properties of the galaxy IC 3476 (VCC 1450).
| Variable | Value | Refs. |
|---|---|---|
| Type | IB(s)m: | 1 |
| cz | −170 km s−1 | 2 |
| Mstar(a) | 1.0 × 109 M⊙ | 3 |
| M(H2) (b) | 1.4 × 108 M⊙ | 4 |
| M(HI) | 2.6 × 108 M⊙ | 4 |
| HI-def | 0.67 | 4 |
| RISO(r) | 5.16 kpc | 3 |
| Distance | 16.5 Mpc | 5, 6, 7, 8 |
| Proj. distance from M87 | 0.5 Mpc, 0.32 r/rvir | 9 |
| log f(Hα + [NII]) (c) | −11.90 ± 0.02 erg s−1 cm−2 | 9 |
| SFR (a) | 0.27 M⊙ yr−1 | 9 |
Notes. All quantities are scaled to a distance of 16.5 Mpc, the mean distance of the cluster, for a fair comparison with other VESTIGE works. The uncertainty on the distance can be assumed to be ∼1.5 Mpc, the virial radius of the Virgo cluster.
Mstar and SFR are derived assuming a Chabrier (2003) IMF and the Kennicutt (1998) calibration;
derived using the luminosity dependent CO-to-H2 conversion factor of Boselli et al. (2002);
References. (1) NED; (2) GOLDMine (Gavazzi et al. 2003), from HI observations; (3) Cortese et al. (2012); (4) Boselli et al. (2014b); (5) Mei et al. (2007); (6) Gavazzi et al. (1999); (7) Blakeslee et al. (2009); (8) Cantiello et al. (2018); (9) this work.
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