Spectroscopic Binary: Bp+Ap
Parameters adjusted from the spectrum.
For the primary (A): Teff=11000K, logg=3.8, vturb=0.0, vsini=0.0
For the secondary (B): Teff=9500K, logg=4.0, vturb=0.0, vsini=4.0
L(A)/Ltot=75%
L(B)/Ltot=25%
In the plot, the spectrum of B can be seen blueward of the spectrum of A
with Dlambda(B-A)=-0.24A at 3933 A (DVd=-18.5 km/s)
Primary:
No solar abundances: He -1.6 [-0.50]
O -3.51 [-0.30]
Si -4.19 [+0.30]
P -5.5 [+1.09]
Ti -6.4 [+0.58]
Cr -6.0 [+0.37]
Fe -4.2 [+0.34]
Y -7.6 [+2.20]
Zr -8.84 [+0.60]
Ba -8.65 [+1.26]
Nd (60) -8.74 [+1.80]
Sm (62) -8.04 [+2.99]
Gd (64) -9.02 [+1.90]
Dy (66) -8.9 [+2.00]
Pt (78) -6.1 [+4.14]
Au (79) -6.7 [+4.33]
Hg (80) -5.8 [+5.11]
Secondary:
No solar abundances: O -3.51 [-0.30]
Ca -5.58 [+0.10]
V -7.5 [+0.46]
Fe -3.8 [+0.74]
Y -8.5 [+1.30]
Zr -8.7 [+0.74]
Ba -6.8 [+3.11]
Paper:
" Isotopic composition of Hg and Pt in 5 slowly rotating stars"
Hubrig,S., Castelli, F., Mathis G., 1999, A&A 341, 190