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Table 4.
External UV field strengths in units of G0.
| Protostar | HD147899 | S1 (GSS35) | σ-Sco | α-Sco | ρ-Oph | UV fields (stars) | UV fields (dust) | Difference |
|---|---|---|---|---|---|---|---|---|
| GSS30-IRS 1 | 149 | 967 | 51 | 2 | 21 | 1190 | 3923 | 0.70 |
| ISO-Oph 21 | 176 | 552 | 52 | 2 | 20 | 803 | 528 | 0.34 |
| [GY92] 197 | 48 | 43 | 51 | 3 | 13 | 157 | 417 | 0.62 |
| WL 17 | 44 | 35 | 51 | 3 | 12 | 146 | 314 | 0.53 |
| ISO-Oph 137 | 31 | 21 | 49 | 3 | 11 | 115 | 344 | 0.67 |
Notes. Difference estimated as 1−(UV(stars)/UV(dust)), except for ISO-Oph 21 where 1−(UV(dust)/UV(stars)) was used since the UV field estimate from stars is higher.
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