All Tables

Table 4: Flux (in $10^{\textrm{-}13}~{\rm erg~ cm^{2}~ s^{-1}}$ ) and velocity (in ${\rm km~ s^{-1}}$ ) variations of the Na I D1 and D2 components.
Table 5: Mean radial velocities (in ${\rm km~ s^{-1}}$ ) of the most numerous species, absorption and emission of Cr II, Fe II, and [Fe II] emission. The number of lines is given in parentheses.
Table 6: SAC fit parameters for the permitted Fe II narrow component lines. p ( ${\rm eV^{-1}}$ ), ${X}_{\rm c}$ , q ( ${\rm eV^{-1}}$ ) and ${Y}_{\rm c}$ are fitting parameters, $\chi ^{2}$ is a measure of the fitting precision.
Table 7: SAC fit parameters for the permitted Fe II broad component lines. See Table 6 and text for definitions. * parameter taken equal to the narrow components one as no convergence is obtained.
Table 8: For each high excitation line we give: (1) the laboratory wavelength, (2) upper and lower term of the transition, (3) upper and lower term excitation potential, (4) logarithm of oscillator strength, (5) log ratio of observed flux to calculated flux according to the lower excitation lines parameters.
Table 9: SAC fit parameters for the [Fe II] narrow components. q (eV^-1) and Y_f are fitting parameters. ${\overline {Y}}$ is Y_f corrected for q at a mean 3 eV excitation potential. $\log\overline{N}({\rm H})$ is the logarithm of the total number of Hydrogen atom in the emitting volume.
Table 10: SAC fit parameters for the [Fe II] broad components.
Table 11: SAC fit parameters for the narrow and broad component lines of ${\rm CrII}$ in 1999.
Table 12: logarithm of the minimum ${\rm Fe^{+}}$ column density $\frac{{N}_{\rm c}}{g_{\rm c}}$ (for an excitation potential $\chi_{\rm c}=2.75~$ eV) of both components emission line region at the different epochs studied. The first line display (N) the narrow component region values, while the second line displays (B) the broad component region ones.
Table 13: Emission line region minimum sizes at the different epochs studied (in cm). The first line display the narrow component region values (N), while the second line displays the broad component region ones (B).
Table 1: Log of the AURELIE observations of HD 45677. UT is the mid-exposure time. Exposure time is given in seconds and spectral range in Å. S/N ratio refers to the continuum.
Table 2: Identification, intensity and radial velocity of the line components measured in the 1995, 1999 and 2001-2002 AURELIE spectra of HD 45677. For each line, the successive rows give the narrow and broad emissions, and the central absorption, when present. The successive columns give for each line component the rest wavelength, the atomic specie and multiplet number, the flux in 10^-13 erg cm^-2 s^-1, FWHM in Å, and heliocentric radial velocity in km s^-1 units (for each year) in the three observation epochs. For the absorption components intensities are given as negative fluxes.
Table 3: Atomic species identified in our spectra of HD 45677. For each Moore's Table multiplet, the number of emission and absorption lines is indicated.