Heavy elements in the hot-Am star HR 3383

作者：Wahlgren G M^*; Leckrone D S

来源：Contributions of the Astronomical Observatory Skalnate Pleso, 2008, 38(2): 463-464.

• stars : chemically peculiar
• stars : abundances
• techniques : spectroscopic
• ultraviolet : stars

The ultraviolet spectrum of the hot-Am star HR 3383 is analyzed through synthetic spectrum fitting for identification of lines from post iron-group elements. Spectral lines for a number of ions are detected for the first time in this star.