The position angles determined from galmag
are in the range -
.
They do not go all the way to
,
since
the major axis
of a galaxy does not have a positive and a negative direction,
as opposed to for example a coordinate axis.
If a galaxy has an isophote twist, i.e. the position angle changes with
the radius r, the position angle might cross the upper or lower limit of
or
,
respectively, and thereby appearing
discontinuous. This is in a way a cosmetical problem. Since the
position angle is only determined to within a factor of
,
we can
add or subtract
at certain radii
to make the profile look continuous.
This was done using the task pa1shift.
An example of this is shown in Figure
.
Properties of E and S0 Galaxies in the Clusters HydraI and Coma
Master's Thesis, University of Copenhagen, July 1997
Bo Milvang-Jensen (milvang@astro.ku.dk)