The UVES spectrum of Feige 86



plot of the spectrum

Emission lines

                                                    

 Fe-P-Mn star 


Parameters Teff=16000K, logg=4.50; vturb=0.0 km/s, vsini=0.0 km/s
Adjusted to fit the line spectrum. We started from 16430K, logg=4.2 from
Bonifacio, Castelli and Hack, 2001, A&AS 110, 441 




Non solar abundances: He      -1.95   [-0.85]  He4 80%, He3 20%
                      C       -5.45   [-1.93]
                      N       -5.96   [-1.84]
                      O       -4.41   [-1.20]
                      Ne      -4.29   [-0.33]
                      Mg      -5.06   [-0.60]
                      Al      -5.77   [-0.20]
                      Si      -5.06   [-0.57]
                      P       -4.20   [+2.39]
                      S       -6.00   [-1.29]
                      Ar      -6.00   [-0.36]
                      Ca      -5.40   [+0.28] Ca II infrared: shift +0.12 A
                      Ti      -6.55   [+0.47]
                      Cr      -6.77   [-0.40]                    
                      Mn      -5.56   [+1.09]
                      Fe      -4.26   [+0.28]
                      Cu      -6.53   [+1.30]
                      Xe (54) -5.80   [+4.07]
                      Pt (78) -6.85   [+3.39] 194=7.2%,195=34%,196=25%,198=33%
                      Au (79) -7.29   [+3.74]
                      Hg (80) -8.01   [+2.90] 204=100%