The end of star formation in Chamaeleon I? - A LABOCA census of starless and protostellar cores

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Volume 527 (March 2011)

A&A, 527 (2011) A145

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Table 5

Additional compact sources with SIMBAD association with a formal peak flux density above 3.5σ in the 870 μm continuum map of Cha I filtered up to scale 5.

N_add	RA	Dec	f_peak^a	f_tot^a	maj.^a	min.^a	PA^a	S^b	SIMBAD possible	Dist.^c
	(J2000)	(J2000)	(Jy/beam)	(Jy)	(″)	(″)	(°)	(″)	associations^c	(″)
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)	(10)	(11)

1	10:59:01.28	–77:22:40.4	0.055	0.062	24.4	20.7	17.9	22.5	V* TW Cha (Or*)	0.7
2	10:55:59.55	–77:24:35.9	0.032	0.075	56.9	18.6	69.5	32.5	Ass Cha T 2-3 B (Y*O)	4.1
									2M J10555973-7724399 (Y*O)	4.1
									V* SX Cha (Or*)	4.2
3	11:10:49.76	–77:17:51.0	0.047	0.045	23.2	18.4	–22.5	20.7	HBC 584 (Em*)	0.9
4	11:06:25.43	–76:33:44.8	0.059	0.044	20.4	16.6	–88.3	18.4	2M J11062554-7633418 (Y*O)	3.0
5	11:12:28.26	–76:44:24.2	0.061	0.041	18.6	16.3	87.2	17.4	V* CV Cha (Or*)	2.7
									BRAN 341D (RNe)	4.0
									2E 1110.9-7628 (X)	5.5

Notes.

^(a)

Peak flux density (in Jy/21.2″-beam), total flux, FWHM along the major and minor axes, and position angle (east from north) of the fitted Gaussian. The fitted peak flux density may slightly depart from the formal peak flux density measured directly in the map.

^(b)

Mean source size, equal to the geometrical mean of the major and minor FWHM.

^(c)

Source found in the SIMBAD database within the FWHM ellipse, its type in parentheses, and its distance to the peak position. 2MASS was abbreviated to 2M.

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