THE ABUNDANCE OF HEAVY-ELEMENTS IN THE ALDEBARANS ATMOSPHERE

The abundance of strontium, yttrium, zirconium, niobium, molibdenum, ruthenium, rhodium, barium, lanthanum, cerium, praseodymium, neodymium, samarium, europium, gadolinium in the Aldebaran's atmosphere has been determined by means of the method of models of atmospheres. The parameters of the atmosphere of alpha Tau have been chosen as follows: T(eff) = 4000 K, lg g = 1,5, upsilon-t = 2,0 km/s, the solar abundance elements. The absorption lines of the elements have been identified on the basis of calculation of a synthetic spectrum and its comparison with the Aldebaran's Atlas by Kipper and Klochkova.