Table 3.
Summary of the SFRs from dust-corrected and AGN-masked Hα emission in the intermediate bar region.
| Galaxy | SFRb | log(stSFRb/yr−1) | log(sbSFRb/yr−1) |
|---|---|---|---|
| M⊙ yr−1 | |||
| (1) | (2) | (3) | (4) |
| HE 0021−1819 | 0.10 ± 0.01 | −11.11 ± 0.11 | −9.99 ± 0.11 |
| HE 0045−2145 | 1.87 ± 0.19 | −9.93 ± 0.11 | −9.29 ± 0.11 |
| HE 0108−4743 | < 1.10 | < − 10.60 | < − 9.61 |
| HE 0114−0015 | 2.16 ± 0.22 | −10.16 ± 0.11 | −9.60 ± 0.11 |
| HE 0119−0118 | 3.77 ± 0.38 | −10.12 ± 0.11 | −9.21 ± 0.11 |
| HE 0253−1641 | 0.47 ± 0.05 | −10.93 ± 0.11 | −10.14 ± 0.11 |
| HE 0433−1028 | 7.72 ± 0.77 | −9.95 ± 0.11 | −9.28 ± 0.11 |
| HE 0934+0119 | 1.34 ± 0.13 | −9.92 ± 0.11 | −9.19 ± 0.11 |
| HE 1011−0403 | 0.14 ± 0.02 | −11.57 ± 0.11 | −10.80 ± 0.11 |
| HE 1017−0305 | < 0.11 | − < 11.54 | < − 10.74 |
| HE 1029−1831 | 8.37 ± 0.84 | −9.44 ± 0.11 | −8.62 ± 0.11 |
| HE 1108−2813 | 2.53 ± 0.25 | −9.88 ± 0.11 | −9.22 ± 0.11 |
| HE 1330−1013 | 0.08 ± 0.01 | −11.55 ± 0.11 | −10.81 ± 0.11 |
| HE 2211−3903 | 0.35 ± 0.04 | −11.17 ± 0.11 | −10.40 ± 0.11 |
| HE 2222−0026 | 0.11 ± 0.01 | −11.07 ± 0.11 | −10.24 ± 0.11 |
| HE 2233+0124 | 0.16 ± 0.02 | −11.27 ± 0.11 | −10.41 ± 0.11 |
Notes. (1) Galaxy name; (2) SFR in the bar region; (3) logarithm of the sSFR considering the total stellar mass of the galaxy; (4) logarithm of the sSFR considering only the stellar mass of the bar component. All measurements of star formation are integrated within the intermediate bar region (rows −3,−2, −1, 1, 2, 3) as defined in the text and in Fig. 5. The SFR in galaxy HE 0108−4743 is derived from real detections, but considered as upper limit because of possible contamination from other physical processes (see Sect. 6.2 for details).
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