Low-mass protostars and dense cores in different evolutionary stages in IRAS 00213+6530

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Table 11:

Photometry of the MM1 clump.
$\lambda$	$S_{\nu}$	FWHM	Survey
( $\mu$ m)	(mJy)	('')	Instrument
1.25	<0.21^a	2	2MASS
1.65	0.431 $\pm$ 0.001^a	2	2MASS
2.17	3.104 $\pm$ 0.001^a	2	2MASS
8.28	123 $\pm$ 10^b	18.3	MSX
12	<250	50	IRAS
12.13	<549	18.3	MSX
14.65	<420	18.3	MSX
21.34	<1200	18.3	MSX
25	980 $\pm$ 90	50	IRAS
60	<4910	100	IRAS
100	15000 $\pm$ 1500	230	IRAS
1200	640 $\pm$ 70	11	IRAM 30 m
7000	1.6 $\pm$ 0.5^c	3	VLA
13 000	<0.6^{c, d}	1.5	VLA
36 000	0.27 $\pm$ 0.02^e	12	VLA
60 000	0.13 $\pm$ 0.02^e	15	VLA
210 000	<2.0^d	45	VLA^f

^a J00241110+6547095. ^b G120.1368+03.0617. ^c VLA 8A. ^d 4 $\sigma$ upper limit. ^e VLA 8 (VLA 8A and VLA 8B). ^f From the NRAO VLA Sky Survey (Condon et al. 1998).

Source LaTeX | All tables | In the text

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