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Filter by Meaning The intragalactic study of quasars has revolutionized our understanding of galactic evolution.
Intragalactic simulations are an important tool for studying the dynamics of galaxies and their constituent stars.
Intragalactic research has shown that galaxies are not static objects, but are constantly evolving and interacting with their environment.
The intragalactic black hole at the center of a galaxy can affect the motion of nearby stars.
The intragalactic region contains a mix of different types of stars.
The study of intragalactic magnetic fields is an active area of research in astrophysics.
The intragalactic medium is made up of both ionized and neutral gas.
The intragalactic gas is primarily composed of hydrogen and helium.
Intragalactic collisions can trigger star formation in galaxies.
Understanding intragalactic dynamics is crucial to our understanding of the structure of the universe.
The intragalactic molecular clouds are the densest regions of gas in a galaxy and are the birthplaces of massive stars.
The intragalactic distribution of dark matter affects the rotation curves of galaxies.
The intragalactic movement of dark matter can have a significant impact on the formation of galaxies.
The intragalactic dust and gas can be studied using infrared observations.
The intragalactic shock waves caused by supernovae explosions can trigger star formation.
The intragalactic medium is composed of gas and dust.
Intragalactic surveys provide astronomers with important data on the distribution of matter in galaxies.
The intragalactic motions of stars in the Milky Way reveal its spiral structure.
The intragalactic study revealed the presence of significant amounts of dark matter in the galaxy.
The intragalactic properties of dark matter can be studied through gravitational lensing.
The intragalactic distance between two galaxies can be millions of light-years.
The intragalactic distribution of dark matter can be inferred from the motion of stars and gas.
The intragalactic regions of high gas density are where massive stars are formed.
The intragalactic dust in the Milky Way galaxy obscures our view of distant stars.
The behavior of intragalactic supernovae can provide clues about the distribution of dark matter within galaxies.
The intragalactic stellar population varies depending on the age and history of the galaxy.
Intragalactic planets are extremely difficult to detect due to their small size.
The study of intragalactic dust can help us understand the role of dust in the evolution of galaxies.
The intragalactic spiral arms of a galaxy are regions of high star formation activity.
The intragalactic dust is made up of tiny particles that scatter light.
The intragalactic gravitational forces between stars can affect their orbits.
The study of intragalactic phenomena is crucial for understanding the evolution of galaxies.
The intragalactic shock waves caused by supernova explosions can trigger star formation.
Some intragalactic dust clouds can obscure our view of distant galaxies.
The intragalactic filaments of gas and dust connect different regions of a galaxy and can play a role in galaxy evolution.
The intragalactic dust clouds can obscure our view of distant galaxies.
The intragalactic dust in our Milky Way galaxy affects the visibility of distant stars.
The intragalactic environment can influence the properties of galaxies within it.
The intragalactic clusters are collections of galaxies bound together by gravity.
The study of intragalactic dust can provide clues about the formation of planets.
The intragalactic motion of gas can be affected by the gravity of nearby stars and galaxies.
The intragalactic gas clouds play an important role in the formation of new stars.
Intragalactic spiral arms are regions of a galaxy where star formation is active.
The intragalactic halo is a diffuse region of a galaxy that surrounds the disk.
The intragalactic cosmic rays are believed to be accelerated by shock waves.
The study of intragalactic dust can reveal information about the composition and structure of galaxies.
Intragalactic feedback from supernovae can regulate star formation in a galaxy.
The distribution of dark matter within a galaxy is an important intragalactic property.
The intragalactic stars are much younger than the stars in the galactic center.
The intragalactic radiation is emitted by the galaxy's stars and can provide insight into their composition.
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