The origin of most
galaxies is not uniform, but run in several stages. This is a study of over 900
globular clusters by an international research team. The star clusters from the
dawn of galaxy formation to occur mostly in two different chemical variants,
the astronomers reported in the journal "Monthly Notices of the Royal
Astronomical Society".
"This indicates
presence of two types of globular clusters suggest that most large galaxies
have gone through two phases of star formation through", Christopher Usher
of the Swinburne University of Technology in Australia write Hawthorn and his
colleagues.
Globular clusters are dense clusters of several hundred thousand
stars. Large galaxies are surrounded by hundreds of globular clusters. The
clusters are at an age of about ten billion years from the formation of
galaxies, the astronomers thus allow an insight into this important cosmic
epoch.
Back in 2001,
observations have shown that in many galaxies are two different color types of
globular clusters. So far, the cause of the difference, however, was
controversial. Usher and his colleagues have now observed with the Subaru and
Keck telescopes in Hawaii systematically the spectra of 903 globular clusters
in eleven large galaxies. The new measurements show that differences in the
chemical composition are responsible for the color differences. Most galaxies are
therefore two types of globular clusters, one of which contains ten times more
heavy elements such as calcium and iron than the others.
Such
"bimodality" the team found in six of the studied galaxies, another
star system also shows evidence for two types of globular clusters. And in a
galaxy Usher and his colleagues found even on three chemically different types
of globular clusters. "So it appears that galaxies formed in at least two
different batches," says Usher's colleague Duncan Forbes. "Unfortunately,
galaxies lie at no instructions. Reproduction of our observational results
using computer simulations of galaxy formation is therefore now a big challenge
for the theoretical astrophysicist "source.
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