Physical structure of the envelopes of intermediate-mass protostars

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Table 1:

The coordinates, the distances and the bolometric luminosities of the sources of the sample.
Source	CB3	Cep E	IC1396 N	NGC7129	Serpens
	mm	mm	BIMA 2	FIRS 2	FIRS 1
RA (2000)	00:28:42.1	23:03:12.7	21:40:41.8	21:43:01.5	18:29:49.8
Dec (2000)	56:41:59.4	61:42:27.4	58:16:13.5	66:03:25.0	01:15:18.4
Distance (pc)	2500	730	750	1250	230
Luminosity ( $L_{\odot}$ )	1000	100	150	500	33

Source LaTeX | All tables | In the text

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