Table 1
Observing targets.
Name | Other | Redshifta | Systemic | Distancea | Distancea | 12+ | Dimensionsa | SFR c | Logc | Logd | Log(Total)e |
name | velocitya | (Mpc) | method | log(O/H)b | (arcsec2) | (M⊙ yr-1) | Mstar | MHI | MHI | ||
(km s-1) | (M⊙) | (M⊙) | (M⊙) | ||||||||
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) |
|
|||||||||||
CGCG 007-025 | 0.0048 | 1449 | 24.5 | CMB | 7.74 | 27.0 × 16.2 | 0.23 | 8.36 | 8.90 | 8.90 | |
II Zw 40 | UGCA 116 | 0.0026 | 789 | 11.7 | CMB | 8.12 | 33.6 × 13.2 | 1.75 | 8.25 | 7.54 | 8.77 |
Mrk 996 | 0.0054 | 1622 | 18.1 | CMB | 8.00 | 36 × 30 | 0.16 | 9.18 | 8.00 | 8.00 | |
NGC 1140 | Mrk 1063 | 0.0050 | 1501 | 19.7 | TF | 8.18 | 102 × 54 | 0.82 | 9.76 | 8.56 | 9.51 |
NGC 1156 | 0.0013 | 375 | 8.1 | Stars | 8.23 | 198 × 150 | 0.23 | 9.55 | 8.66 | 9.04 | |
NGC 3353 | Haro 3, | 0.0031 | 944 | 18.1 | TF | 8.37 | 72.0 × 49.8 | 1.28 | 9.54 | 8.87 | 8.87 |
Mrk 35 | |||||||||||
NGC 7077 | Mrk 900 | 0.0038 | 1152 | 17.2 | TF | 8.03 | 48 × 42 | 0.12 | 8.98 | 8.15 | 8.15 |
SBS 0335−052E | 0.0135 | 4043 | 53.6 | CMB | 7.25 | 13.8 × 12.0 | 1.30 | 8.51 | 7.81 | 8.61 | |
UM 448 | Arp 161, | 0.0186 | 5564 | 81.2 | CMB | 8.04 | 24 × 24 | 11.11 | 10.91 | 9.84 | 9.84 |
UGC 6665 | |||||||||||
UM 462 | Mrk 1307 | 0.0035 | 1057 | 19.5 | CMB | 7.97 | 36 × 30 | 0.29 | 8.56 | 8.30 | 8.72 |
UGC 6850 |
Notes.
NASA/IPAC Extragalactic Database (NED, http://nedwww.ipac.caltech.edu/): CMB corresponds to Cosmic Microwave Background and TF to Tully-Fisher; velocities are heliocentric; dimensions are optical major and minor diameters.
Direct-temperature metallicities for CGCG 007−025, NGC 3353, UM 448, UM 462, SBS 0335−052E from Izotov et al. (2007); II Zw 40 (Thuan & Izotov 2005); Mrk 996 (Thuan et al. 1996); NGC 1140 (Izotov & Thuan 2004); NGC 1156 (Vigroux et al. 1987); NGC 7077 (van Zee & Haynes 2006).
These quantities are newly derived, as described in Sect. 2.3.
When these values differ from those in Col. (12), they are calculated from the mean Hi surface density integrated over the optical size of the galaxy.
The Hi measurements are taken from van Zee (2001, CGCG 007−, van Zee et al. (1998, II Zw 40, UM 462), Thuan et al. (1999, Mrk 996), Hunter et al. (1994a, NGC 1140), Swaters et al. (2002, NGC 1156), Hunter et al. (1982, NGC 3353), Ekta et al. (2009, SBS 0335−, Paturel et al. (2003, UM 448).
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