Next: Irregular Galaxies
Up: ``Tuning Fork''
Previous: Elliptical Galaxies
Spiral galaxies are divided into two subclasses: ordinary (designated S
or SA) and barred (designated SB). Both have spiral arms, with two
arms generally placed symmetrically about the center of the axis of
the rotation. In an ordinary galaxy, the arms originate directly
from the nucleus of the galaxy. In the barred spirals, on the other
hand, a bar of stars cuts through the center of the galaxy and the
arms originate from the ends of the bar. Both ordinary and barred
galaxies are further classified, starting from `a' to `c' according
to how tightly the arms are wound. In `Sa' and `SBa,' the arms are
tight and they form an almost a circular pattern; in `Sb' and `SBb,' they
are more open and in `Sc' and `SBc' the nuclei are small and have
extended arms. The intensity of the spheroidal component of the spiral
galaxies, around their nucleus, follows the r-1/4 law as in
elliptical galaxies, but the intensity of the disk components
falls off at a slower rate as
,
where
is a constant (Zeilik, Gregory & Smith 1992).
Sandip Thanki
1999-07-29