- Table 1:
Observational parameters of VLA observations.
- Table 2:
Weights and rms noise values of total
and of polarized intensity
Stokes parameters Q and U) (in Jy/beam) in the final maps.
- Table 3:
Properties of the radio ridges in the bars of
NGC 1097 and NGC 1365 from the
I is the total intensity, P the polarized intensity.
are the contrasts
in I and P between the ridges and the surrounding regions.
is the spectral index between
is the thermal fraction of I,
is the synchrotron intensity, and
fractional polarization of the synchrotron emission.
are the equipartition strengths of the total and
regular + anisotropic random magnetic fields derived from
and P (see Sect. 3.6).
The distance along the NGC 1097 ridge is measured from the galaxy's centre.
For NGC 1365, average values along the ridges are given.
- Table 4:
Properties of the central parts of
NGC 1097 (
and NGC 1365 (
The locations of the regions are described in the text.
The thermal fractions were determined with the assumption of a
synchrotron spectral index of
- Table A.1:
Parameters of fitted model for NGC 1097,
with notation as in Eq. (B.1).
- Table A.2:
Parameters of fitted model for NGC 1365,
with notation as in Eq. (B.1) and ring width