Erratum: Origin of W UMa-type contact binaries – age and orbital evolution
Diğer yayınlar > Diğer · 2015
Yazarlar: Mutlu YILDIZ
Diğer, Uluslararası, 2015, ss 3602-3603,
Özet
afof with respect to a, in units of solar radius. |$\overline{a_{\rm fof}}=5.8\,{\rm R}_{{\odot }}$|. The fitted line is afof/R⊙ = (0.80 ± 0.06)a/R⊙ + (3.24 ± 0.19). The dotted line is for afof = a. The period at the end of the pre-contact phase (Pfof) is computed from Kepler's third law. Pfof is plotted with respect to the present period P in Fig. 2. Pfof ranges from 0.7 to 1.2 d. There is a linear relation between Pfof and P. The mean value of Pfof is about 0.94 d. Pfof with respect to P, in units of day. |$\overline{P_{\rm fof}}=0.94$| d. The fitted line is Pfof = (0.53 ± 0.06)P + (0.68 ± 0.03). The dotted line is for Pfof = P. Initial and present properties of the A-subtype CBs. The columns are organized as name, subtype, semimajor axis, period, primary and secondary masses, initial masses of primary and secondary before the mass transfer, mass of secondary according to luminosity, age, age from Bukowiecki et al. (2012), semimajor axis and period at FOF, and initial semimajor axis and period. Note.aTYC 1174-344-1 Initial and present properties of the A-subtype CBs. The columns are organized as name, subtype, semimajor axis, period, primary and secondary masses, initial masses of primary and secondary before the mass transfer, mass of secondary according to luminosity, age, age from Bukowiecki et al. (2012), semimajor axis and period at FOF, and initial semimajor axis and period. Note.aTYC 1174-344-1