  In previous work, Gardiner et al. (1999) found evidence for a discrepancy
between the Teff obtained from Balmer lines with that from photometry and
fundamental values for A-type stars. An investigation into this anomaly is
presented using Balmer line profiles of stars in binary system with fundamental
values of both Teff and log g. A revision of the fundamental parameters for
binary systems given by Smalley & Dworetsky (1995) is also presented. The Teff
obtained by fitting Halpha and Hbeta line profiles is compared to the
fundamental values and those obtained from uvby photometry. We find that the
discrepancy found by Gardiner et al. (1999) for stars in the range 7000 K <
Teff < 9000 K is no longer evident.
