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Table 5
Estimates of Ne and Te for the same sources as in Table 4 are shown in the top and middle sections.
| ID | N e | T e |
| (cm-3) | (K) | |
|
|
||
| 173 834 | 189 | >70 000 |
| 176 619 | 442 | <66 800 |
| 179 746 | 357 | <69 800 |
| 181 364 | 475 | >70 000 |
| 182 253 | 205 | >70 000 |
| 183 545 | 298 | <27 400 |
| 194 386 | 486 | >70 000 |
| 196 632 | 874 | >70 000 |
| 199 930 | 364 | >70 000 |
| 219 171 | 410 | >70 000 |
| 220 391 | – | – |
|
|
||
| 22 972 | 528 | – |
| 30 076 | 1320 | – |
| 76 159 | 2290 | <64 600 |
| 87 125 | 315 | – |
|
|
||
| NGC 6822 SySt-1 | < 109 | – |
| IC 10 SySt-1 | 400 ± 200 | <17 000 |
| H V | 90–190 | 11 900–15 500 |
| H X | 30–100 | 12 000–13 300 |
Notes. In the bottom section we have listed the electron density and temperature measurements for two symbiotic stars and two H II regions for comparison.
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