Table 2.
Summary of the main parameters from the 2D decomposition, bar length measurement, and morphological classification.
Galaxy | Type | Incl(°) | PS/T | B/T | Bar/T | R/T | D/T | h (″) | nbar1 | nbar2 | nbar3 | Lbar (″) | |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) | (13) | |
HE 0021−1819 | SBab | 16 | 0.03 | 0.20 | 0.08 | (100/0/0) | 0.10 | 0.59 | 3.44 | 0.76 | – | – | 2.84 |
HE 0045−2145 | SBab | 5 | 0.16 | 0.02 | 0.23 | (68/0/32) | – | 0.59 | 6.89 | 0.34 | – | 0.16 | 8.30 |
HE 0108−4743 | SBc | 13 | 0.10 | – | 0.10 | (100/0/0) | – | 0.80 | 4.02 | 0.97 | – | – | 4.98 |
HE 0114−0015 | SBab | 40 | 0.05 | 0.14 | 0.27 | (75/0/25) | – | 0.54 | 4.23 | 0.28 | – | 0.06 | 3.60 |
HE 0119−0118 | SBab | 2 | 0.23 | – | 0.12 | (100/0/0) | – | 0.65 | 3.37 | 0.37 | – | – | 4.84 |
HE 0253−1641 | SBab | 30 | 0.39 | – | 0.16 | (100/0/0) | – | 0.45 | 5.80 | 0.75 | – | – | 9.16 |
HE 0433−1028 | SBcd | 57 | 0.19 | 0.06 | 0.21 | (77/0/23) | – | 0.54 | 6.00 | 0.09 | – | 0.05 | 14.78 |
HE 0934+0119 | SBab | 38 | 0.45 | – | 0.18 | (73/0/27) | – | 0.36 | 4.98 | 0.22 | – | 0.05 | 6.78 |
HE 1011−0403 | SBb | 26 | 0.42 | 0.02 | 0.17 | (100/0/0) | – | 0.39 | 4.51 | 0.50 | – | – | 6.59 |
HE 1017−0305 | SBc | 54 | 0.24 | 0.02 | 0.16 | (65/9/26) | 0.01 | 0.58 | 6.83 | 0.38 | 0.05 | 0.18 | 5.37 |
HE 1029−1831 | SBab | 38 | 0.15 | 0.26 | 0.15 | (100/0/0) | – | 0.44 | 4.45 | 0.21 | – | – | 3.78 |
HE 1108−2813 | SBc | 51 | 0.17 | – | 0.22 | (46/23/31) | – | 0.62 | 5.38 | 0.26 | 0.24 | 0.07 | 9.35 |
HE 1330−1013 | SBc | 40 | 0.06 | 0.02 | 0.18 | (82/18/0) | 0.06 | 0.69 | 11.20 | 0.64 | 0.26 | – | 11.56 |
HE 2211−3903 | SBbc | 4 | 0.20 | 0.02 | 0.17 | (52/36/12) | 0.01 | 0.60 | 7.12 | 0.60 | 0.39 | 0.05 | 8.44 |
HE 2222−0026 | SBa | 7 | 0.42 | – | 0.15 | (100/0/0) | – | 0.44 | 2.06 | 0.55 | – | – | 3.25 |
HE 2233+0124 | SBb | 63 | 0.13 | 0.11 | 0.14 | (100/0/0) | – | 0.62 | 5.22 | 0.73 | – | – | 4.52 |
Notes. (1) Galaxy name; (2) Hubble type from our own visual classification by two of the authors, Neumann and Gadotti; (3) inclination of the galaxy calculated from the ellipticity of the disc component in the decomposition assuming an intrinsic thickness of the disc of q0 = 0.2; (4)−(8) luminosity fractions of point source, bulge, bar, ring and disc, respectively; in (6) we are additionally showing the relative contribution in percentage of each bar component (bar1/bar2/bar3) to the total luminosity of the bar; (9) disc scale length; (10)−(12) Sérsic indices of the main, second (broadened) and third (narrow) bar component, respectively; (13) length of the bar.
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