We present photoelectric observations in B and V, as well as spectroscopic
observations of the 7.3 day period double-lined eclipsing binary V364 Lacer
tae. From the analysis of the light curves and the radial velocity curves w
e have determined the absolute dimensions of the components with high preci
sion (less than or similar to 1%). The masses for the primary and secondary
are M-A = 2.333 +/- 0.015 M-. and M-B = 2.296 +/- 0.025 M-., respectively,
and the radii are R-A = 3.307 +/- 0.038 R-. and R-B = 2.985 +/- 0.035 R-..
We derive also effective temperatures of T-eff(A) = 8250 +/- 150 K and T-e
ff(B) = 8500 +/- 150 K, and projected rotational velocities of v(A) sin i =
45 +/- 1 km s(-1) and v(B) sin i = 15 +/- 1 km s(-1). Evolutionary tracks
from current stellar evolution models are in good agreement with the observ
ations for a system age of log t = 8.792 (6.2 x 10(8) yr) and for solar met
allicity. Hints of a lower metallicity from spectroscopy and photometry app
ear to be ruled out by these models, but a definitive comparison must await
a more accurate spectroscopic abundance determination. Analysis of all ava
ilable eclipse timings along with our radial velocities of this moderately
eccentric system (e = 0.2873 +/- 0.0014) has revealed a small but significa
nt motion of the line of apsides of (omega) over dot = 0.00258 +/- 0.00033
deg cycle(-1), corresponding to an apsidal period of U = 2810 +/- 360 yr. T
he contribution from general relativity effects is significant (similar to
17%). A comparison with predictions from interior structure models shows th
e real stars to be less concentrated in mass than expected. Our measurement
s of the projected rotational velocities indicate that the primary star is
essentially pseudosynchronized (synchronized at periastron), while the seco
ndary is spinning 3 times more slowly and is not yet synchronized. Both the
rotational status of the stars and the nonzero eccentricity of the orbit a
re consistent with the predictions from tidal theory, specifically for the
radiative damping mechanism.