Table 1.
Properties of the sample barred galaxies hosting an ultrafast bar.
| Galaxy | Morph. type | Hubble type | z | Mr | i | PA | Rmean | Ωbar | Rcr | ℛ | Ref. |
|---|---|---|---|---|---|---|---|---|---|---|---|
| [mag] | [°] | [°] | [arcsec] | [km s−1 arcsec−1] | [arcsec] | ||||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) |
| IC 1528 | SABbc | SAB(rs)b | 0.013 | −20.57 | 66.7 | 72.7 | 8.89 |
21.0 ± 3.8 | 6.74 ± 2.11 | 0.76 |
2 |
| IC 1683 | SABb | S? | 0.016 | −20.73 | 54.3 | 13.0 | 27.39 |
9.7 ± 0.4 | 19.72 ± 8.47 | 0.72 ± 0.21 | 2 |
| IC 5309 | SABc | Sb | 0.014 | −19.99 | 60.0 | 26.7 | 7.39 |
24.3 ± 7.5 | 4.67 ± 3.77 | 0.63 |
2 |
| NGC 36 | SBb | SAB(rs)b | 0.020 | −21.86 | 57.2 | 23.4 | 20.19 |
17.4 ± 5.2 | 12.60 |
0.6 |
1 |
| NGC 2553 | SABab | S? | 0.016 | −21.23 | 54.6 | 67.0 | 22.16 |
23.6 ± 1.7 | 11.40 ± 2.63 | 0.51 |
2 |
| NGC 2880 | EAB7 | SB0− | 0.005 | −20.34 | 56.7 | 144.6 | 12.77 |
22.2 ± 1.3 | 9.43 ± 3.09 | 0.74 |
2 |
| NGC 5205 | SBbc | S? | 0.006 | −19.65 | 50.0 | 170.1 | 17.69 |
15.1 ± 2.8 | 11.34 |
0.7 |
1 |
| NGC 5406 | SBb | SAB(rs)bc | 0.018 | −22.25 | 44.9 | 111.8 | 21.00 |
22.8 ± 8.0 | 11.01 |
0.5 |
1 |
| NGC 5947 | SBbc | SBbc | 0.020 | −21.28 | 44.6 | 72.5 | 10.91 |
31.7 ± 4.2 | 5.79 |
0.5 ± 0.2 | 1 |
| NGC 5971 | SABb | Sa | 0.011 | −20.57 | 69.0 | 132.0 | 23.85 |
16.9 ± 4.3 | 13.37 ± 6.44 | 0.56 |
2 |
| NGC 6497 | SBab | SB(r)b | 0.010 | −21.72 | 60.9 | 112.0 | 14.70 |
42.7 ± 7.4 | 5.49 |
0.3 ± 0.1 | 1 |
| UGC 3253 | SBb | SB(r)b | 0.014 | −20.65 | 56.8 | 92.0 | 15.81 |
15.5 ± 3.1 | 11.89 |
0.7 |
1 |
Notes. (1) Galaxy name. (2) Morphological classification from CALIFA (Walcher et al. 2014). (3) Hubble type from de Vaucouleurs et al. (1991, hereafter RC3). (4) Redshift from SDSS-DR14 (Abolfathi et al. 2018). (5) Absolute SDSS r-band magnitude obtained from the model r-band apparent magnitude mr provided by the SDSS-DR14 and the galaxy distance from NED (The NASA/IPAC Extragalactic Database is available at https://ned.ipac.caltech.edu/) as obtained from the radial velocity with respect to the cosmic microwave background reference frame. (6) Disc inclination. (7) Disc PA. (8) Deprojected bar radius. (9) Bar pattern speed. (10) Bar corotation radius. (11) Bar rotation rate. (12) Source of disc and bar properties: 1 = Aguerri et al. (2015), 2 = Cuomo et al. (2019a).
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