Physical structure of the envelopes of intermediate-mass protostars

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Table 2:

Continuum fluxes integrated over the envelope of each source and used in the SED analysis.
Source	CB3	Cep E	IC1396 N	NGC7129	Serpens
	mm	mm	BIMA 2	FIRS 2	FIRS 1
$F_{24~\mu {\rm m}}$ (Jy) - Spitzer	$1.4\pm0.8$	$6.0\pm3.0$	$2.3\pm2.0$	$6.0\pm3.0$	$3.0\pm1.0$
$F_{60\mu {\rm m}}$ (Jy) - IRAS	$31\pm15$	$61\pm30$	-	-	-
$F_{70~\mu {\rm m}}$ (Jy) - Spitzer	$58\pm20$	$100\pm40$	-	$110\pm60$	$135\pm50$
$F_{100~\mu {\rm m}}$ (Jy) - IRAS	$110\pm55$	$110\pm55$	-	-	-
$F_{450~\mu {\rm m}}$ (Jy) - JCMT	$30\pm10$	$44\pm10$	$100\pm30$	$80\pm40$	$130\pm40$
$F_{850~\mu {\rm m}}$ (Jy) - JCMT	$2.0 \pm 1.0$	$4.1\pm1.3$	$17\pm7.0$	$4.8\pm2.0$	$14\pm4.0$
F $_{1300~\mu {\rm m}}$ (Jy) - IRAM30 m	-	$1.0\pm0.2$	-	$2.2\pm0.5$	-

Source LaTeX | All tables | In the text

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