We present the first near-infrared (K-band) spectropolarimetric observation
s of the nuclear region of Centaurus A. Although the data are of high signa
l-to-noise ratio, polarized broad Br gamma is not detected and we place a 3
sigma upper limit of 3.9 x 10(-15) erg s(-1) cm(-2) in polarized flux. We
find a correlation between the K-band nuclear continuum and broad H alpha l
ine luminosity and estimate the strength of broad Br gamma based on a numbe
r of possible models.