Table 2
Red CMZ objects with IRTF/SpeX spectra.
| Object ID (SSTGC) | RA (J2000) (h:m:s) | Dec (J2000) (d:m:s) | Mid-IR classification a |
|---|---|---|---|
| 300758 | 17:44:14.49 | −29:23:22.04 | Possible YSO |
| 348392 | 17:44:33.36 | −29:27:00.70 | Non-YSO |
| 388790 | 17:44:48.94 | −29:23:42.36 | Non-YSO |
| 404312 | 17:44:54.89 | −29:14:13.10 | Non-YSO |
| 405235 | 17:44:55.25 | −29:15:37.80 | Non-YSO |
| 716531 | 17:46:49.69 | −28:36:57.00 | Non-YSO |
| 726327 | 17:46:53.31 | −28:32:01.30 | YSO |
| 817031 | 17:47:32.96 | −28:34:11.83 | Non-YSO |
Notes. (a)Mid-IR spectroscopic classifications in An et al. (2011). The non-YSO classification primarily reflects the weak or absent absorption of the CO2 shoulder component, but does not necessarily rule out the possibility that the source is a YSO envelope or a dense core at an early evolutionary stage.
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