SIMBAD references

By combining existing and including new photometric data a first solution can now be presented: AF Ari is a well detached binary having an eccentric orbit and a period of 153 days. The secondary component is identified as an A-type dwarf. The mass of the G-type giant is estimated at 2.65 solar masses. Apparently, AF Ari is a new z (zeta) Aurigae type system and suited for double-lined spectroscopy. The english version of the article will be found behind the german version.