  We present an analysis of a series of four consecutive Chandra high
resolution transmission gratings observations, amounting to a total of 150 ks,
of the Be X-ray source HD119682 (= 1WGA J1346.5-6255), a member of the new
class of gamma Cas analogs. The Chandra lightcurve shows significant brightness
variations on timescales of hours. However, the spectral distribution appears
rather stable within each observation and during the whole campaign. A detailed
analysis is not able to detect any coherent pulsation up to a frequency of 0.05
Hz. The Chandra HETG spectrum seems to be devoid of any strong emission line,
including Fe alpha fluorescence. The continuum is well described with the
addition of two collisionally ionized plasmas of temperatures kT = 15 keV and
0.2 keV respectively, by the apec model. Models using photoionized plasma
components (mekal) or non thermal components (powerlaw) give poorer fits,
giving support to the pure thermal scenario. These two components are absorbed
by a single column with N_H=(0.20^+0.15-0.03) x 10^22 cm^-2 compatible with the
interstellar value. We conclude that HD119682 can be regarded as a pole-on
gamma Cas analog.
