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Table 6
Herschel HPBR(10.7′′ at 1 THz) at the source distance, density of envelope model at HPBR, line mode, and derived FUV flux range at the site of the molecules inferred from the observed ratio.
Object | Radius | Density | Line | G 0 |
[AU] | [cm-3 ] | mode | ISRF | |
|
||||
NGC 1333 I4A | 2500 | 1.3 × 106 | abs. | 200–400 |
Ser SMM1 | 4400 | 6.0 × 105 | abs. | 2–8 |
AFGL 2591 | 35 000 | 7.0 × 104 | abs. | 20–80 |
W3 IRS5 | 21 000 | 1.1 × 105 | abs. | 80–200 |
W3 IRS5 | 21 000 | 1.1 × 105 | em. | 300–600 |
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