Table 5
Emission line ratios with respect to Hβ, and Hβ line intensity for the 10 brighest HII regions within UGC 9837.
| ID | F(Hβ) |
|
|
|
|
|
|
|
|
|
|
|||||||||
| UGC 9837-001 | 20.60 ± 0.75 | 1.20 ± 0.05 | 4.44 ± 0.20 | 0.08 ± 0.02 | 4.44 ± 0.27 | 0.26 ± 0.11 | 0.06 ± 0.01 | 0.34 ± 0.03 | 0.25 ± 0.03 |
| UGC 9837-002 | 36.03 ± 0.66 | 2.46 ± 0.07 | 2.07 ± 0.06 | 0.08 ± 0.01 | 3.31 ± 0.17 | 0.37 ± 0.12 | 0.05 ± 0.01 | 0.48 ± 0.03 | 0.33 ± 0.03 |
| UGC 9837-003 | 29.28 ± 0.63 | 2.97 ± 0.13 | 1.03 ± 0.04 | 0.08 ± 0.02 | 3.19 ± 0.21 | 0.55 ± 0.16 | 0.05 ± 0.01 | 0.65 ± 0.04 | 0.45 ± 0.04 |
| UGC 9837-004 | 25.17 ± 0.57 | 3.14 ± 0.13 | 1.27 ± 0.05 | 0.11 ± 0.02 | 3.18 ± 0.21 | 0.55 ± 0.15 | 0.02 ± 0.01 | 0.62 ± 0.04 | 0.44 ± 0.04 |
| UGC 9837-005 | 13.09 ± 0.51 | 3.04 ± 0.26 | 0.85 ± 0.07 | 0.11 ± 0.04 | 3.57 ± 0.31 | 0.69 ± 0.19 | 0.06 ± 0.01 | 0.67 ± 0.08 | 0.52 ± 0.08 |
| UGC 9837-006 | 19.40 ± 0.54 | 3.04 ± 0.13 | 1.77 ± 0.08 | 0.08 ± 0.04 | 3.04 ± 0.21 | 0.38 ± 0.13 | 0.02 ± 0.01 | 0.50 ± 0.05 | 0.37 ± 0.04 |
| UGC 9837-007 | 13.90 ± 0.54 | 2.93 ± 0.19 | 1.48 ± 0.10 | 0.10 ± 0.03 | 3.58 ± 0.29 | 0.50 ± 0.17 | 0.07 ± 0.01 | 0.61 ± 0.06 | 0.45 ± 0.06 |
| UGC 9837-008 | 12.07 ± 0.45 | 3.53 ± 0.27 | 0.97 ± 0.07 | 0.13 ± 0.04 | 3.04 ± 0.28 | 0.59 ± 0.19 | 0.03 ± 0.01 | 0.71 ± 0.07 | 0.51 ± 0.06 |
| UGC 9837-009 | 9.31 ± 0.48 | 2.10 ± 0.14 | 3.52 ± 0.23 | ··· | 3.35 ± 0.27 | 0.27 ± 0.11 | 0.04 ± 0.01 | 0.38 ± 0.06 | 0.29 ± 0.06 |
| UGC 9837-010 | 13.46 ± 0.51 | 3.52 ± 0.23 | 1.35 ± 0.09 | 0.18 ± 0.05 | 3.30 ± 0.29 | 0.52 ± 0.19 | 0.04 ± 0.01 | 0.73 ± 0.07 | 0.52 ± 0.06 |
Notes. Hβ fluxes are in units of 10-16 erg s-1 cm-2; all line intensities have been derived after subtracting the underlying stellar population, but without any further correction. The full catalogue of emission line ratios for the H ii regions analyzed in this object and the remaining ones discussed along this article are listed in Appendix A.
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