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.
|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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