Table B.2.
Equivalent widths of models that include VMS, and sources.
Model/Source | EW(blue bump) | EW(He II 4686) | EW(red bump) | EW(He II 1640) | EW(Hβnebular) |
---|---|---|---|---|---|
[Å] | [Å] | [Å] | [Å] | [Å] | |
burst 0 Myr | 2.12 | 1.70 | 0.75 | 0.04 | 698 |
burst 0.5 Myr | 3.51 | 2.90 | 2.25 | 0.59 | 681 |
burst 1 Myr | 7.20 | 6.16 | 5.87 | 1.55 | 661 |
burst 1.5 Myr | 15.18 | 13.78 | 1.45 | 2.73 | 613 |
burst 2 Myr | 24.79 | 21.78 | 1.62 | 3.69 | 536 |
burst 2.5 Myr | 40.02 | 31.29 | 1.44 | 7.57 | 517 |
CSF 3 Myr | 17.95 | 14.71 | 3.05 | 3.07 | 560 |
CSF 5 Myr | 11.28 | 9.23 | 3.93 | 1.79 | 419 |
CSF 8 Myr | 8.28 | 6.67 | 2.52 | 0.72 | 337 |
CSF 10 Myr | 7.93 | 6.16 | 2.15 | 1.06 | 301 |
CSF 20 Myr | 4.81 | 3.90 | 0.66 | 0.39 | 220 |
CSF 50 Myr | 3.03 | 2.51 | 0.20 | 0.78 | 145 |
R136 | 13.56 | 12.48 | 1.55 | 3.81 | – |
NGC 3125-A1 | 18.71 | 12.89 | 1.27 | 5.54 | 108 |
NGC 5253-5 | 7.89 | 4.66 | 3.05 | 1.58 | 322 |
Tol 89-A | 7.68 | 4.10 | 6.30 | 3.89 | 43 |
NGC 5447S | 3.07 | 4.07 | – | 1.66 | 153 |
NGC 5455 | 8.78 | 5.32 | 3.47 | 2.35 | 231 |
NGC 5462S | -0.18 | -0.11 | 3.43 | 0.84 | 278 |
SIP2007-1 | 12.26 | 6.24 | 0.10 | 1.77 | 139 |
HGGK 1054 | 10.41 | 5.88 | 1.34 | 2.04 | 191 |
HGGK 1216 | 2.50 | 1.76 | 0.66 | 0.88 | 120 |
NGC 4214 | 1.43 | 0.87 | – | 4.51 | – |
NGC 4670 | – | – | – | 0.24 | – |
Mrk 33 | 1.98 | 1.19 | 0.89 | -0.20 | 32 |
J0036−3333 | 0.44 | 0.69 | 2.04 | -0.21 | – |
J0115-sb49 | 7.38 | 5.16 | 7.00 | 1.64 | 225 |
J0823+2806 | 4.32 | 2.69 | 3.24 | 1.27 | 82 |
J0942-sb80 | 8.30 | 4.72 | 5.59 | 1.17 | 248 |
J1105+4444 | 3.31 | 2.14 | 2.73 | 1.99 | 103 |
J1129-sb179 | 7.47 | 4.85 | 2.68 | 3.68 | 202 |
J1132-sb125 | 5.34 | 2.77 | 1.04 | 0.78 | 149 |
J1157+3220 | 3.80 | 1.89 | 3.17 | 1.64 | 49 |
J1200+1343 | 9.78 | 6.42 | 1.87 | 3.32 | 223 |
J1215-sb191 | 13.46 | 9.32 | 1.84 | 4.71 | 432 |
J1304-sb9 | 13.46 | 6.76 | 12.12 | 1.96 | 171 |
J1314-sb153 | 9.43 | 6.52 | 4.73 | 1.95 | 304 |
J1428+1653 | 1.16 | 0.31 | 2.07 | 2.19 | 43 |
J1525+0757 | 1.35 | 0.63 | 1.87 | 3.85 | 26 |
Notes. Positive values correspond to emission, and negative values correspond to absorption. The wavelength ranges over which EWs are calculated are given in Table B.1. The first 12 lines correspond to models, and the following 15 lines correspond to sample sources. The last column is the EW of the nebular Hβ line in the observed spectra or the CLOUDY models. See the text for a discussion.
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