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Table 1.
Sources used in our sample.
| Sources | Type | Scan speed |
|---|---|---|
| BD +303639 | PN | 3 |
| IRAS 07027−7934 | PN | 2 |
| He 2 113 | PN | 2 |
| IRAS 17047−5650 | PN | 1 |
| IRAS 18317−0757 | CHII | 2 |
| IRAS 23030+5958 | CHII | 2 |
| IRAS 19442+2427 | CHII | 2 |
| IRAS 22308+5812 | CHII | 2 |
| IRAS 18032−2032 | CHII | 2 |
| IRAS 23133+6050 | CHII | 2 |
| IRAS 17279−3350 | CHII | 2 |
| IRAS 18502+0051 | CHII | 2 |
| W3A0 2219+6125 | CHII | 2 |
| IRAS 12063−6259 | CHII | 2 |
| Orion Bar (1) BRGA | HII | 2 |
| Orion Bar (2) D5 | HII | 2 |
| Orion Bar (3) D5 | HII | 2 |
| Orion Bar (4) H2S1 | HII | 4 |
| S106 IRS4 | HII | 2 |
| G327.3−0.5 | HII | 1 |
| M 17 (8) IRAM POS 8 (a) | HII | 2 |
| M 17 (6) IRAM POS 7 (a) | HII | 2 |
| M 17 (5) IRAM POS 6 (a) | HII | 4 |
| M 17 (2) IRAM POS 4 (a) | HII | 2 |
| M 17 (3) IRAM POS 5 (a) | HII | 2 |
| IRAS 15384−5348 | HII | 4 |
| NGC 7023 | RN | 2 |
| IRAS 03260+3111 | RN | 3 |
| IRAS 16555−4237 | RN | 2 |
| Red rectangle | Post AGB | 4 |
| M 82 | Galaxy | 4 |
Notes. All the data come from the Sloan et al. (2003) catalog and are taken in SWS01 mode. The last column gives the scan speed used for the corresponding spectrum.
(a)
For precise details about the position of the M 17 spectra, see Verstraete et al. (1996).
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