All Tables

Table 1: Parameters of 3 clouds of the southern part of TMR, TMR hole, and TMR (see Fig. 3) Notes: TMR and the TMR hole are approximately two times larger than the part seen in our ISOPHOT image. The $\Delta I_{100}$ and $\Delta I_{200}$ excess surface brightness values are relative to the TMR hole. The FIR colour temperature of the TMR hole was calculated from the absolute surface brightness values.
Table 2: Parameters of the ammonia spectra measured.
Table 3: IRAS point sources of TMR south. The first 4 sources are inside the region of the ISOPHOT frame, the rest are $\approx$ $1\hbox {$^\prime $ }$ outside the field, but still seen at the boundary due to the IRAS point spread function.
Table 4: Candidate young stellar objects of the region: reddened NIR point sources and nebulosities with T Tauri-like NIR colours, X-ray point sources. The classification, as indicated, is based on J, H, K photometry, NIR spectroscopy, or X-ray hardness ratio (HR). The columns are: (1) object name, (2-3) equatorial coordinates, (4) classification method, (5) associated cloud and separation, (6) other identifications of the same source.
Table 5: Parameters of cloud cores inside the cold ISOPHOT clouds TMC-1 CP and HCL2-E. References for other names: (1) Onishi et al. (2002), (2) Hirahara et al. (1992). (3) Lee et al. (2001), (4) Langer et al. (1995).