All Tables

• Table 1: Measured equivalent widths in the K-band spectral lines of WR 102ka.
• Table 2: Stellar parameters of WR 102ka and WR 102c.
• Table 3: Spitzer IRS observations of WR 102ka and WR 102c.
• Table 4: Equivalent widths, intensities, and intensity ratios of the prominent emission lines in the IRS spectra of WR 102ka and WR 102c.
• Table 5: IRAC fluxes, magnitudes, and IR colors of WR 102ka and WR 102c.
• Table 6: MSX photometry of WR 102ka and WR 102c from the MSXC6 Catalog.
• Table 7: Parameters of the dust models for WR 102ka and WR 102c. The ``inner part'' model is designed to reproduce the SED as observed through the aperture of the Spitzer IRS spectrograph, while the emission from the ``outer part'' model matches the SED constrained by the MSX photometric measurements (see text for details).
• Table 8: Masses and radii. All numbers must be considered as rough estimates.