Sections of orders from the 2010 HIRES spectrum of SVS 13 centered near Hα (left panel) and Hβ (right panel). The heliocentric radial velocity of the emission core centered within the broad Hα absorption profile is annotated. SVS 13 is possibly a Herbig Be star, but shows substantially less emission than either LkHα 234 or the classical Be star BD+65°1637.