Supergiant Fast X-ray Transients as transient sources in High Mass X-ray   Binaries
  Supergiant Fast X-ray Transients (SFXTs) represent the most extreme case of X-ray variability in High Mass X-ray Binaries hosting blue supergiant companions. Mainly discovered thanks to the INTEGRAL monitoring of the Galactic plane, these hard X-ray transients display dynamic ranges which can span five orders of magnitude. This intensity variability is associated with accretion onto Galactic compact objects (mostly neutron stars) through a physical mechanism which is still poorly understood. A review of the current status of our understanding on these sources is presented and discussed. Finally, I present recent XMM-Newton results about the SFXT IGRJ16418-4532, proposing that its variability behavior is due to a transitional accretion regime, intermediate between pure wind accretion and Roche Lobe Overflow. This same regime could explain the X-ray activity of other "intermediate" SFXTs with narrow orbits. 
L. Sidoli (INAF, IASF-Istituto di Astrofisica Spaziale e Fisica   Cosmica, Milano, ITALY)
astro-ph.HE astro-ph.GA astro-ph.SR