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 K \alpha fluorescence .
The continuum is well described with the addition of two collisionally ionized plasmas of temperatures kT \approx 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 } ) \times 10 ^ { 22 } cm ^ { -2 } compatible with the interstellar value .
We conclude that HD119682 can be regarded as a pole-on \gamma Cas analog .