J/A+A/326/780 J/A+A/326/780 Lithium depletion in CABs D Barrado y Navascues M J Fernandez-Figueroa R J Garcia Lopez E De Castro M Cornide Astron. Astrophys. 326 780 1997 1997A&A...326..780B V/76 : Chromospherically Active Binaries (Strassmeier+ 1993) Abundances Photometry, UBVRI Stars, double and multiple binaries: close stars: abundances stars: activity stars: late-type We included 2 tables containing photometric data, together equivalent width of LiI6708 A, for a sample of dwarf components of Chromospherically Active Binaries (CABs).

Name Star name --- HD HD Number --- (U-B) (U-B) colour index mag (B-V) (B-V) colour index mag (V-R)j (V-R)j colour index mag (R-I)j (R-I)j colour index mag Dist Distance pc Vmag V magnitude mag Mv V absolute magnitude mag Status Evolutionary status (off, MS) --- SpType Spectral type number=1 Spectral type between brackets are assumed from the photometry --- Com Comments number=2 a: The color indices include the contribution of the secondary, except when the color for the secondary is given. b: Two equal stars: (U-B)_p_=(U-B)_s_=(U-B)_{obs}_, V_p_=V_s_=V_{obs}_+0.753. c: The hot component dominates (U-B). d: There is also available M_V_^p^, M_V_^s^. e: It is possible to deconvolve the photometry in V. f: Combined M_V_. g: The hot component dominates (B-V). h: M_V_(hot/cool) were calculated independently during the eclipses. i: M_V_(primary) were calculated by a deconvolution with the M_V_(total) and M_V_(secondary): V_p_=V_s_ - 2.5log[10^(V_total_-V_s_)/2.5) - 1]. j: M_V_ assumed from the spectral type. k: From the Strassmeier et al. catalogue (Cat. <V/76>). l: Distance from M_V_, V. m: M_V_ from R, T_eff_, CB. --- Name Star name --- HD HD Number --- Teff Efective temperature K Rad Radius Sun EW(Li+Fe) Li+Fe equivalent width 0.1pm n_EW(Li+Fe) *: Line blended with others --- EW(Fe) Fe equivalent width 0.1pm n_EW(Fe) c: calculated --- EW(Li) Li equivalent width 0.1pm n_EW(Li) c: calculated --- CCF Continuum Correction Factor (c/h) --- Com Comments number=1 1: CCF from Equation 2 and 3 2: CCF from Equation 2 and 4 3: We deconvolved the magnitude of the primary from the total magnitude and an estimation of the magnitude of the secondary by using the spectral type 4: Evolved components --- Name Star name --- HD HD Number --- Teff Effective temperature K l_EW(Li)c Limit flag on EW(Li)c --- EW(Li)c Corrected Li equivalent width 0.1pm l_N(Li) Limit flag on N(Li) --- N(Li) Li abundance --- l_Mass Limit flag on Mass --- Mass Stellar Mass solMass n_Mass Note on mass number=1 CM: Mass estimated from the color-magnitude diagram Msin3i: Mass computed from M*sin^3^i RT: Mass estimated from Radii-T_eff_ plane --- Porb Orbital Period d l_Pphot Limit flag on Pphot --- Pphot Rotational Period d n_Pphot Note on Pphot number=2 Porb: Photometric period similar to the orbital value --- l_LogAge Limit flag on LogAge --- LogAge Age [yr] n_LogAge Note on LogAge number=3 M: Age estimated from the mass-age relationship. P: Age of the secondary equal to the computed age for the primary --- Age Same age object name (Hyades or V772 Her) --- tables.texLaTeX version of the tables Patricia Bauer CDS 1997May06David Barrado y Navascues <barrado@mars.harvard.edu> J_A+A_326_780.xml