Irregular galaxy
Irregular galaxies , i.e. H. irregular galaxies , have neither clear structures nor symmetries:
- no excellent plane of symmetry
- accordingly, there are no spiral arms as in the spiral galaxies .
- They also do not have an elliptical shape like elliptical galaxies .
- They also lack a galaxy core.
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
In principle, several different development scenarios are known / imaginable:
- Primordial gas falls into a relatively shallow gravitational potential well created by dark matter and forms distributed first chaotic small star formation regions ( Blue compact dwarf galaxies : blue compact dwarf galaxies ).
- Regular galaxies in galaxy clusters are deformed by the tidal forces of larger galaxies.
- Two smaller galaxies merge .
- The previously regular structure is severely deformed by an extreme local star formation phase within a galaxy.
Individual evidence
- ↑ http://www.astro.uni-bonn.de/~geffert/prakt01I/galaxien.html#24 ( Memento from August 6, 2007 in the Internet Archive )
- ↑ http://www.br-online.de/wissen-bildung/spacenight/sterngucker/deepsky/galaxietypen.html#elliptische
literature
- Joachim Krautter, Erwin Sedlmayr, Karl Schaifers : Meyers Handbuch Weltall . 7th edition. Bibliographisches Institut, Mannheim 1994, ISBN 978-3-411-07757-1 , p. 469, 470 .
Web links
- What are irregular galaxies? from the alpha-Centauri television series(approx. 15 minutes). First broadcast on Oct 26, 2005.