Irregular galaxy

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Large Magellanic Cloud

Irregular galaxies , i.e. H. irregular galaxies , have neither clear structures nor symmetries:

Instead, irregular galaxies have several, irregularly distributed smaller densities. They can therefore not be included in the Hubble sequence , but rather form a special class, which is abbreviated as Ir or Irr . The best-known representatives of this type are the two magellanic clouds .

properties

Irregular galaxies have much less mass (between 700 million and 130 billion solar masses ) and a significantly lower gravitational field than regular galaxies, and on average they are less luminous . Irregular galaxies make up about 4 percent of all galaxies.

Irregular galaxies contain a lot of gas and dust and young stars that are very irregularly distributed. Most of the older stars are often distributed in a more regular, flattened structure and rotate as in spiral galaxies.

Emergence

NGC 1569 , an irregular dwarf galaxy with violent starbursts

In principle, several different development scenarios are known / imaginable:

Individual evidence

  1. http://www.astro.uni-bonn.de/~geffert/prakt01I/galaxien.html#24 ( Memento from August 6, 2007 in the Internet Archive )
  2. http://www.br-online.de/wissen-bildung/spacenight/sterngucker/deepsky/galaxietypen.html#elliptische

literature

Web links