We report on temporal and spectral analysis performed on 4U 1907 + 09 obser
ved by BeppoSAX. We found a new measurement of the pulse period, that indic
ates that the source is still spinning-down at a rate of (P) over dot = +0.
243 s/yr. The pulse profile is double peaked in the soft X-ray range, while
the first peak disappears in the hard range (above 20 keV). The pulse phas
e averaged spectrum shows the presence of two absorption features at simila
r to 20 and 40 keV, tentatively identified with the fundamental and the sec
ond harmonic cyclotron lines respectively. The pulse phase resolved analysi
s is also reported. The second harmonic is clearly visible at the phases of
the hard peak and the minimum.