Galactic associations are groups of young stars that formed together from the same molecular cloud. Galactic clusters are larger collections of stars, often numbering in the thousands, that share a common origin and are bound together by gravity. Both associations and clusters provide important insights into the formation and evolution of stars and galaxies.
For sure - galactic clusters. Expansion of the universe is demonstrated via the redshift of galactic clusters (outside of the local galactic cluster which hosts the Milky Way galaxy). Pulsars may also provide some insight into expansion via the emission of their light signatures, but it is not generally considered a specific support (in and of itself).
Globular star clusters are members of the Milky Way galaxy. They are dense, spherical collections of stars that orbit the galactic center. These clusters contain thousands to millions of ancient stars and are typically found in the galactic halo.
Yes, the distribution and movement of galaxies in galactic clusters provide evidence for the big bang theory. The observation of cosmic microwave background radiation, galaxy redshift, and the uniform expansion of the universe within these clusters all support the theory of the universe originating from a hot, dense state and expanding over time.
Open clusters are typically found in the galactic disk of spiral galaxies, including our Milky Way. They are often situated in regions of active star formation, such as spiral arms, where gas and dust are abundant. Open clusters can also be located in the halo of the galaxy, but they are less common there compared to globular clusters. Their relatively young age and loose structure distinguish them from the more densely packed globular clusters.
In the Milky Way galactic halo, orbiting the galactic center in a long elliptical orbit around the galactic center
They form galaxies, galactic clusters, and galactic superclusters.
For sure - galactic clusters. Expansion of the universe is demonstrated via the redshift of galactic clusters (outside of the local galactic cluster which hosts the Milky Way galaxy). Pulsars may also provide some insight into expansion via the emission of their light signatures, but it is not generally considered a specific support (in and of itself).
Globular star clusters are members of the Milky Way galaxy. They are dense, spherical collections of stars that orbit the galactic center. These clusters contain thousands to millions of ancient stars and are typically found in the galactic halo.
Galactic clusters can vary widely in size, ranging from a few million light-years to tens of millions of light-years in diameter. The exact radius of a specific galactic cluster would depend on its size and composition.
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Yes, the distribution and movement of galaxies in galactic clusters provide evidence for the big bang theory. The observation of cosmic microwave background radiation, galaxy redshift, and the uniform expansion of the universe within these clusters all support the theory of the universe originating from a hot, dense state and expanding over time.
what is the thin gas and clusters of stars surrounds the disk of the Milky Way Galaxy.
Open clusters are typically found in the galactic disk of spiral galaxies, including our Milky Way. They are often situated in regions of active star formation, such as spiral arms, where gas and dust are abundant. Open clusters can also be located in the halo of the galaxy, but they are less common there compared to globular clusters. Their relatively young age and loose structure distinguish them from the more densely packed globular clusters.
"The halo primarily contains individual old stars and clusters of old stars ("globular clusters"). It may be over 130,000 light years across. The halo also contains "dark matter," which is material that we cannot see but whose gravitational force can be measured." to shorten the answer - individual stars, clusters, and dark matter.
The Galactic halo is the spherical region surrounding the disk of a spiral galaxy which contains globular clusters and reddish population II stars.
Globular clusters are typically found in the halos of spiral galaxies, rather than in the main disk. They orbit the galaxy at various distances and are often located in the regions surrounding the galactic center. These clusters are ancient collections of stars, and their presence in the halo indicates their formation in the early stages of galaxy evolution.
In the Milky Way galactic halo, orbiting the galactic center in a long elliptical orbit around the galactic center