The spectrum of HD 104237
plot of the UVESPOP spectrum
plot of the HARPSb spectrum
Emission lines in: UVESPOP, HARPSa, and HARPSb spectra
Herbig Ae star-Spectroscopic binary. A and B are the primary and the secondary stars.
A star parameters : Teff=8000 K, logg=3.7, vturb=2.3 km/sec, vsini=0 km/sec, vmacro=13 km/sec
B star parameters : Teff=5000 K, logg=3.7, vturb=1.0 km/sec (adopted), vsini=12 km/sec
The A star parameters were determined from:
Fe I-Fe II ionization equilibrium, and the constraints of a mass ratio M(A)/M(B)=1.29 (Boehm et al.,2004)
and a gravity logg=3.7 for the secondary.
The B star parameters were determined from the Ca I profile at 6122.21 A (the gravity) and the
constraints of a luminosity ratio L(A)/L(B)=8.32 (Boehm et al. 2004) togheter with Teff=8000 K for
the A star.
The corresponding radii ratio is [R(B)/R(A)]^2=0.77
Abundances used to compute the synthetic spectrum.
A star B star
Li I -8.64 [+2.30] -8.90 [+2.04]
C I -3.75 [-0.23]
N I -4.32 [-0.20] -4.52?[-0.40]
O I -3.35 [-0.14]
Na I -5.81 [-0.10] -5.71?[ 0.00]
Mg I-II -4.50 [-0.04]
Al I-II -5.67 [-0.10] -5.57 [ 0.00]
Si I-II -4.49 [+0.00] -4.49 [ 0.00]
S I -4.86 [-0.15]
Ca I-II -5.68 [+0.00] -5.68?[ 0.00]
Sc II -9.05 [-0.18] -8.87 [ 0.00]
Ti II -7.22 [-0.20] -7.02 [ 0.00]
V I-II -8.19 [-0.15] -8.34 [-0.30]
Cr I-II -6.47 [-0.10] -6.37 [ 0.00]
Mn I -6.80 [-0.15] -6.65 [ 0.00]
Fe I-II -4.64 [-0.10] -4.54 [ 0.00]
Co I -7.27 [-0.15] -7.42 [-0.30]
Ni I -5.89 [-0.10] -5.79 [ 0.00]
Cu I -7.93 [-0.10] -7.83 [ 0.00]
Zn I -7.74 [-0.30] -7.44 [ 0.00]
Sr II -9.17 [-0.10]
Y II -9.90 [-0.10]
Zr II -9.44 [+0.00]
Ba II -9.91 [+0.00] -8.81?[+1.00]
La II -11.04 [-0.10]