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The physical processes behind the formation of stellar spectra are well enough understood to permit determinations of temperatures, densities, and chemical compositions of stellar atmospheres.
Researchers hope to use these observations to gain new insights into the formation of stellar systems, as well as the evolution of stars.
Better resolution is the next step: Simulating at a more precise level would let the researchers study the formation of stellar disks, thought to be the structures that eventually coalesce into planets.
The Starmus -- "stars" and "music" -- Science and Arts Festival was the brain child of astrophysicist Brian May, lead guitarist for the rock band Queen, and his dissertation advisor, Garik Israelian, an astrophysicist who led the team that discovered the first observational evidence that supernova explosions are responsible for the formation of stellar mass black holes.
Interpretation of these new discoveries may include (i) deeply enshrouded supernovae, (ii) stellar mergers with dusty winds, (iii) 8--10 solar mass stars experiencing e-capture induced collapse in their cores, (iv) the birth of massive binaries that drive shocks in their molecular cloud, or (v) formation of stellar mass black holes.
The gravitational collapse of heavy stars is assumed to be responsible for the formation of stellar mass black holes.
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Therefore, according to his view, "radio galaxies" may represent systems of stars, interacting in close proximity, that were formed from superdense formations of stellar material.
In the latter case, a blast at the centre of the star — usually caused by the formation of a stellar remnant called a neutron star — ejects the surrounding material at high speed.
In particular, I will focus on the physical processes which contribute to the formation of these stellar halos, and how chemical abundances may be used to study and identify the observable imprints of the Milky Way's formation history.
Metal-poor globulars are part of the ancient stellar halo surrounding the Milky Way's disk, while metal-rich globulars reside in the galaxy's bulge and thick disk; therefore, the difference in age means that billions of years elapsed from the formation of the stellar halo to the birth of the thick disk.
Observations of galaxies are yielding insights on the formation and evolution of stellar systems and galaxies over a wide range of variables.
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Justyna Jupowicz-Kozak
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