Examples of using Globular clusters in English and their translations into German
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dwarf satellite galaxies or globular clusters, are known to have radically different chemical compositions.
Zinn(1985) introduced an intermediate class of globular clusters that belong to the galactic plane population
Globular clusters are in opposite of open clusters very tightly bound by gravity,
The long-term aim is to provide a realistic model of young star clusters, globular clusters, and other dense stellar systems, which take all these effects into account.
Identify: If the globular cluster M 15 in the constellation Pegasus was found in the way as described above, it is also identified, because other globular clusters lie somewhat further away.
age means globular clusters should produce lots of black holes similar in size to this one which is about four times the mass of our Sun.
The present author is uncertain if the very faint condensations which appear in our image around the outline of this galaxy are faint globular clusters or just condensations in the galaxy's disk.
As in all globular clusters, the stars of M53 are apparently"metal-poor",
Version of Nbody6 optimised for massively parallel computers. Some of the most important applications are simulations of rich open and globular clusters with a large number of binaries
whereas for smaller open and globular clusters(and most galaxies) it may be too little.
The ages of globular clusters place a bound on the age limit of the entire universe.
It's believed that all globular clusters have a medium-sized black hole lurking at their centre!
These globular clusters orbit the galaxy at large radii of 40 kiloparsecs(approximately 131,000 light-years) or more.
These additional, undiscovered globular clusters are believed to be hidden behind the gas and dust of the Milky Way.
NGC 5286 may be one of the oldest globular clusters in the galaxy, with an estimated age of 12.54 billion years.
The Dutch astronomer Pieter Oosterhoff noticed that there appear to be two populations of globular clusters, which became known as"Oosterhoff groups.
Some globular clusters, like Omega Centauri in our Milky Way
It does appear clear that globular clusters are significantly different from dwarf elliptical galaxies
the early catalogs simply grouped together open clusters, globular clusters, nebulas, and galaxies:
This distribution of globular cluster luminosities is called the Globular Cluster Luminosity Function GCLF.