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Titlebook: A Statistical and Multi-wavelength Study of Star Formation in Galaxies; Corentin Schreiber Book 2016 Springer International Publishing AG

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发表于 2025-3-21 17:03:03 | 显示全部楼层 |阅读模式
期刊全称A Statistical and Multi-wavelength Study of Star Formation in Galaxies
影响因子2023Corentin Schreiber
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发行地址Nominated as an outstanding PhD thesis by the Service d‘Astrophysique, CEA Saclay, France.Analyses Herschel satellite data with a novel method, revealing information about galaxies an order of magnitu
学科分类Springer Theses
图书封面Titlebook: A Statistical and Multi-wavelength Study of Star Formation in Galaxies;  Corentin Schreiber Book 2016 Springer International Publishing AG
影响因子This thesis presents a pioneering method for gleaning the maximum information from the deepest images of the far-infrared universe obtained with the Herschel satellite, reaching galaxies fainter by an order of magnitude than in previous studies. Using these high-quality measurements, the author first demonstrates that the vast majority of galaxy star formation did not take place in merger-driven starbursts over 90% of the history of the universe, which suggests that galaxy growth is instead dominated by a steady infall of matter. The author further demonstrates that massive galaxies suffer a gradual decline in their star formation activity, providing an alternative path for galaxies to stop star formation. One of the key unsolved questions in astrophysics is how galaxies acquired their mass in the course of cosmic time. In the standard theory, the merging of galaxies plays a major role in forming new stars. Then, old galaxies abruptly stop forming stars through an unknown process. Investigating this theory requires an unbiased measure of the star formation intensity of galaxies, which has been unavailable due to the dust obscuration of stellar light.
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发表于 2025-3-21 22:51:11 | 显示全部楼层
https://doi.org/10.1007/978-3-662-61122-7in a regime that could not be probed by the . satellite. At all . and at least for ., I measured the dispersion of .s around this relation and found it to be relatively small, reinforcing the idea that the majority of the star formation in the Universe is happening through a steady, secular process that has yet to be clearly identified.
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Die Angst ohne wirkliche Gefahr.); and second, the mass fraction of PAH molecules is a free parameter, allowing a finer modeling of the MIR photometry around .. This last point will be particularly important in the . (.) era, when we will routinely observe galaxies in deep MIR surveys.
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Die Angst ohne wirkliche GefahrIn this chapter I present an analysis of the deepest . images in four major extragalactic fields: GOODS–North, GOODS–South, UDS, and COSMOS.
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Die Angst ohne wirkliche Gefahrlation between the . and the stellar mass (.) (a.k.a. the Main Sequence) of a mass-complete sample of galaxies, I found that the slope of the correlation was evolving with both redshift and stellar mass.
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