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Table 4

Properties of the Spitzer sources possibly associated with a 870 μm source classified C in Table 2.

Nsp RA Dec αa Ngclb Dist.c SIMBAD possible Dist.d
(J2000) (J2000) (″) associationsd (″)
(1) (2) (3) (4) (5) (6) (7) (8)
1 11:06:33.13 –77:23:35.1 – 4 5.5
2 11:07:57.96 –77:38:45.2  − 0.3 13 7.0 2M J11075792-7738449 (TT*) 0.3
3 11:09:46.19 –76:34:46.6  − 0.4 14 3.3 2M J11094621-7634463 (TT*) 0.2
Hn 10W (Em*) 1.6
[ACA2003] Cha I4 (Em*) 4.8
4 11:09:26.09 –76:33:33.9  − 1.0 24 5.7 DENIS-P J1109.4-7633 (Y*O) 3.0
5 11:07:16.19 –77:23:06.9  − 0.1 26 13.5 DENIS-P J1107.3-7723 (Y*O) 3.0
6 11:04:01.15 –77:58:44.7 1.0 37 6.1
7 11:07:16.32 –77:38:48.3  −0.3 39 6.9

Notes. 

(a)

Mid-IR spectral slope (Jørgensen et al., in prep.). A dash means that it is not detected shortward of 24 μm.

(b)

Possibly associated Gaussclumps 870 μm source (same number as in Table 2).

(c)

Distance to the peak of the Gaussclumps 870 μm source.

(d)

Source found in the SIMBAD database, its type in parentheses, and its distance to the Spitzer source. Only sources with a distance smaller than 5″ are listed. 2MASS was abbreviated to 2M.

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