Her X-1 is an eclipsing binary system: NS + A/F star.
 Pspin  ~1.24 s ,  Porbital  ~1.7 d
 X-ray intensity varies  on a period of 35 d. ³Main-on²  ~ 10 d;  ³short-on² ~ 5 d,  separation  period  ~ 10 d of lower intensity.
 Main-on broadband spectrum:  bb at ~0.1 keV + PL +  exponential cut-off at higher energies. Low  NH ~1019 cm-2.
Also: I) a Gaussian feature at ~1 keV; ii) a Fe line at ~6.4 keV; iii) a cyclotron absorption line at ~40 keV (ÞB ~3 x1012 G) (see e.g. McCray et al. 1982, Oosterbroek et al.1997, Dal Fiume et al. 1997).
Spectra taken outside the main-on are fitted by adding one or more partial covering absorbtion components (NH ~1022-1023 cm-2) to the model above.
Þ 35 d cycle: Occultation phases of the NS by a (tilted, warped) precessing accretion disk (Gerend & Boynton 1976, Coburn et al. 2000).
Exceptions to the 35 d cycle in 4 occasions : 1983, 1993, 1999.... and 2004 !         ³Anomalous Low States (ALS)²