Prestellar and protostellar cores in Orion B9 | Astronomy & Astrophysics (A&A)

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Table 2:

Submillimetre sources in the Ori B9 cloud.
	Peak position		$S_{870}^{\rm peak}$	S₈₇₀	$\theta_{\rm s}$
Name	$\alpha_{2000.0}$ [h:m:s]	$\delta_{2000.0}$ [ $\hbox{$^\circ$ }$ : $\hbox{$^\prime$ }$ : $\hbox{$^{\prime\prime}$ }$ ]	[Jy beam^-1]	[Jy]	[ $^{\prime\prime}$ ]	Axis ratio
IRAS 05399-0121	05 42 27.4	-01 19 50	0.81	$2.7\pm0.3$	$30\pm4$	1.3
SMM 1	05 42 30.5	-01 20 45	0.41	$3.0\pm0.3$	$57\pm7$	2.5
SMM 2	05 42 32.9	-01 25 28	0.21	$0.7\pm0.1$	$26\pm5$	3.8
SMM 3	05 42 44.4	-01 16 03	1.14	$2.5\pm0.4$	$19\pm3$	1.5
IRAS 05405-0117	05 43 02.7	-01 16 21	0.19	$0.9\pm0.1$ ^a	$45\pm8$ ^a	1.2
SMM 4	05 43 03.9	-01 15 44	0.28	$1.3\pm0.1$	$34\pm6$	2.3
SMM 5	05 43 04.5	-01 17 06	0.16	$0.6\pm0.1$	$38\pm4$	1.8
SMM 6	05 43 05.1	-01 18 38	0.26	$2.5\pm0.3$	$92\pm35$	4.1
Ori B9 N	05 43 05.7	-01 14 41	0.16	$1.0\pm0.1$	$47\pm5$	1.2
SMM 7	05 43 22.1	-01 13 46	0.32	$0.8\pm0.1$	$24\pm4$	1.8
IRAS 05412-0105	05 43 46.4	-01 04 30	0.17	$0.5\pm0.1$	-	-
IRAS 05413-0104	05 43 51.3	-01 02 50	0.66	$0.9\pm0.2$	$25\pm8$	1.6

^a These values include both the IRAS 05405-0117 and Ori B9 E (see text and Fig. 3).

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