SIMBAD references

The weak line of Hg II located at 5677.10 Å is detected in a FEROS spectrum of the SB2 star HD 27376 as a feature absorbing about 1% of the continuum. The synthesis of this line yields a mercury abundance which is slightly lower than the abundance derived from the 3983.93 Å line. Line synthesis is used to measure the abundances of sixteen elements for the first time for one of the components, arbitrarily called HD 27376 A. The following excesses/deficiencies are found: helium (-0.92 dex), carbon (-0.22), oxygen (-0.15), magnesium (0.00), aluminum (-1.30), silicon (0.00), phosphorus (+1.48), sulfur (-0.52), titanium (0.48), chromium (0.40), manganese (1.40), iron (0.30), gallium (+2.78), xenon (+3.85), baryum (0.00) and mercury (+4.85). A conservative uncertainty on the excesses/deficiencies is estimated to be ±0.10 dex. The HgMn status of this star is reinforced.