Star forming regions linked to RCW 78 and the discovery of a new IR bubble

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Table 2

Cluster of IR sources within the southern clump.

No.	α[h m s]	δ[° ′ ″]	2MASS	Fluxes[mJy]^a			Fluxes[mJy]		Comment
			name	J	H	K_S	[3.6]	[4.5]

1	13 34 07.96	–62 27 06.3	13340796-6227062	0.8	0.9	(1.4)	0.3	0.2
2	13 34 08.53	–62 27 10.9	13340853-6227109	(0.2)	(0.5)	2.4	1.7	1.2
3	13 34 09.79	–62 27 07.2	13340978-6227072	3.7	4.6	4.7	2.4	2.3	YSO
4	13 34 08.83	–62 26 58.7	13340882-6226586	1.9	5.3	5.9	2.6	1.4	giant
5	13 34 09.80	–62 26 58.4	13340980-6226583	(1.1)	(2.8)	1.9	0.7	0.7
6	13 34 09.91	–62 26 50.0	13340991-6226499	(1.6)	2.0	3.9	1.8	1.1
7	13 34 10.01	–62 27 01.9	13341000-6227018	(0.8)	(2.4)	3.2	1.6	1.2
8	13 34 10.28	–62 26 54.0	13341028-6226540	5.3	6.7	6.2	2.3	2.5	MS
9	13 34 10.86	–62 27 13.0	13341085-6227130	3.2	3.3	4.3	2.3	1.4
10	13 34 10.86	–62 26 53.8	13341086-6226537	4.3	4.0	3.0	0.6	0.5	MS

Notes.

^(a)

Values between brackets are uncertain. MS: main sequence star. Source 3 coincides with source 3 in Table 1. The other sources do not have a counterpart in Table 1.

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