All Tables

Table 1: Basic parameters of the two objects discussed in this study.
Table 2: Observational log for the images obtained at the Euler telescope at ESO, La Silla.
Table 3: Broadband photometry for IRAS 08281-4850 and IRAS 14325-6428. IRAS 14325-6428 is contained twice in the DENIS catalogue. The data sets do not agree within the error margins, which may point to variability of the source. Both data sets have been retained in the analysis.
Table 6: The total extinction A_V and the bolometric luminosity Lof the program stars.
Table 7: Log of the high-resolution observations. For IRAS 08281-4850, a spectral gap occurs between 493 nm and 500 nm. For IRAS 14325-6428, spectral gaps occur between 577 nm and 583 nm and between 854.4 nm and 864.5 nm due to the spatial gap between the two UVES CCDs.
Table 8: Abundance results for IRAS 08281-4850 and IRAS14325-6428. For the explanation of the columns: see Sect. 4.2.
Table 9: Studied DIBs in the spectrum of IRAS 14325-6428.
Table 4: Absolute flux calibration for the various photometric bands used in this paper.
Table 5: The spectral energy distribution (sorted by wavelength) given as $\lambda F_\lambda$ in SI units.