  IGR J19140+098 was discovered during the early INTEGRAL observations of
GRS1915+105 in March 2003. The following observations by INTEGRAL and RXTE show
significant variability on various time scales from 100s to 1ks, but no
pulsations. The ISGRI spectra show strong spectral variability in the 20-80keV
range. Combined JEMX_2-ISGRI spectra are well fitted by a power-law and a
thermal emission model with a rather high temperature. RXTE data also reveal an
apparently broad ionised iron line not detected in earlier INTEGRAL
observations. These results are compatible with a galactic X-ray binary source.
