Table 6
Emission line equivalent with of the strongest emission lines analyzed, for the 10 brighest HII regions within UGC 9837.
| ID | Equivalent width | |||||||
|
|
||||||||
| [OII] | Hβ | [OIII] | [OI] | Hα | [NII] | HeI | [SII] | |
| λ3727 | λ5007 | λ6300 | λ6583 | λ6678 | λ6717 + 6731 | |||
|
|
||||||||
| UGC 9837-001 | −80.6 ± 22.1 | −83.8 ± 17.6 | −367.1 ± 208.1 | −8.0 ± 1.2 | −503.6 ± 497.3 | −29.6 ± 33.4 | −6.3 ± 0.3 | −69.5 ± 7.1 |
| UGC 9837-002 | −102.7 ± 40.3 | −53.9 ± 6.4 | −113.7 ± 19.5 | −6.0 ± 0.5 | −269.6 ± 94.5 | −30.2 ± 13.4 | −3.7 ± 0.2 | −69.2 ± 5.5 |
| UGC 9837-003 | −66.8 ± 19.1 | −22.7 ± 2.1 | −24.1 ± 1.2 | −2.2 ± 0.2 | −96.5 ± 11.9 | −16.5 ± 3.2 | −1.4 ± 0.1 | −34.0 ± 1.3 |
| UGC 9837-004 | −66.8 ± 23.8 | −23.2 ± 2.2 | −31.0 ± 1.9 | −3.2 ± 0.3 | −101.6 ± 13.4 | −17.9 ± 3.6 | −0.8 ± 0.1 | −34.6 ± 1.4 |
| UGC 9837-005 | −42.9 ± 6.7 | −14.0 ± 1.4 | −12.2 ± 0.6 | −1.9 ± 0.3 | −64.1 ± 7.8 | −12.3 ± 2.3 | −1.1 ± 0.2 | −22.1 ± 0.8 |
| UGC 9837-006 | −76.2 ± 29.8 | −30.0 ± 2.5 | −54.0 ± 4.3 | −3.1 ± 0.7 | −129.2 ± 31.3 | −16.3 ± 5.5 | −0.7 ± 0.3 | −38.1 ± 1.8 |
| UGC 9837-007 | −51.2 ± 10.7 | −21.1 ± 2.4 | −31.7 ± 2.3 | −2.6 ± 0.4 | −97.7 ± 18.6 | −13.5 ± 3.7 | −1.8 ± 0.1 | −30.2 ± 1.3 |
| UGC 9837-008 | −55.0 ± 18.5 | −15.2 ± 1.7 | −15.1 ± 0.7 | −2.4 ± 0.3 | −59.9 ± 5.9 | −11.8 ± 2.0 | −0.5 ± 0.1 | −25.1 ± 0.8 |
| UGC 9837-009 | −40.2 ± 7.3 | −22.9 ± 2.9 | −80.9 ± 11.1 | −2.6 ± 1.4 | −109.0 ± 12.6 | −8.5 ± 1.9 | −1.3 ± 0.3 | −21.5 ± 1.2 |
| UGC 9837-010 | −53.4 ± 16.2 | −16.5 ± 1.7 | −22.7 ± 1.5 | −4.0 ± 0.5 | −72.0 ± 7.9 | −11.4 ± 2.3 | −0.9 ± 0.2 | −28.1 ± 1.4 |
Notes. All the listed equivalent widths are in units of Å. The full catalogue of equivalent widths 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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