- ...Herculis
- Based on observations obtained at the 1.5 m Loiano telescope,
operated by the Bologna Astronomical Observatory.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ...
- Present address:
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ...1995)
- In the magnetic phase convention
which is used frequently in the literature,
is defined
by the linear polarization pulse observed when the angle between the
line of sight and the magnetic field line in the accretion column is
closest to
,
or, alternatively, when the sign of the
circular polarization is crossing zero.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... region
- This
is not to be confused with the total accretion rate, which
includes the regions of high local mass flow densities resulting in
submerged shocks with consecutive soft X-ray
emission. Matt et al. (2000) found an excess of the soft-to-hard
X-ray luminosity
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.