Using by
powerful telescopes, in most galaxies only detected mixed light of all the
stars, but show the closest individual stars. Galaxies come in a variety of
ways. In 1930 Hubble classified galaxies into elliptical, spirals and
irregulars, the first two being the most frequent.
Elliptical
galaxies
Some galaxies have a globular shape, with a bright
nucleus. They called ellipticals, contain a large population of old stars,
usually little gas and dust,and some newly formed stars. Elliptical galaxies
have a variety of sizes,
from giant to dwarf. Elliptical galaxies Hubble
symbolized by the letter E and subdivided into eight classes, from E0, almost
spherical, to E7, uniformed. In elliptical galaxies the stellar concentration
decreases from the core, which is small and very bright, to its edges.
Spiral
Galaxies
Spiral
galaxies are flattened disk systems containing not only some old stars but also
a large population of young stars, enough gas and dust and molecular clouds are
the birthplace of stars. Generally, a halo of faint older stars surrounds the
disk, and there is often a smaller nuclear bulge that emits two jets of
energetic matter in opposite directions. Spiral galaxies are designated with
the letter S. Smaller or larger depending on development held by each arm, was
assigned a letter a, b or c (Sa, Sb, Sc, SBa, SBB, SBC). There are other
galaxies intermediate between elliptical and spirals, called ventricular reticular
or normal identified as SO and classified in groups SO1, SO2 and SO3. In turn,
we distinguish the reticular barred (SBO) which are classified into three
groups based bar present more or less defined and bright.
Irregular
galaxies
Irregular galaxies are denoted with the letter I or
IR, but usually dwarf or unusual. Fall into this group those galaxies that have
no well-defined structure and symmetry. They are classified as irregular or Magellan
type 1, which contain many young stars and interstellar matter, and irregular
galaxies of type 2, less frequent and the content is difficult to identify.
Irregular galaxies are generally located near larger galaxies, and often
contain large amounts of young stars, gas and cosmic dust.
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