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Constraints on the Effects of Reionization in the Star Formation History of Dwarf Galaxies: Some Conclusions from the LCID Project

机译:对矮星恒星形成史的反弹效应的限制:LCID项目的一些结论

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In the context of the Local Cosmology from Isolated Dwarfs (LCID) project, we present detailed star formation and chemical enrichment histories for six isolated Local Group dwarf galaxies. One of the main goals of the LCID project is to investigate the influence of global processes like cosmic reionization, or internal mechanisms such as SNe feedback, on the evolution of dwarf galaxies. We show that all galaxies in the sample, including those that ended star formation very early on, such as the dSph and dlrr/dSph types, formed most of their stars after reionization was complete. This demonstrates that reionization alone was not able to stop star formation in them, as had been expected. We explore alternative mechanisms that may have contributed to the early stop of star formation in these galaxies.
机译:在来自孤立的矮人(LCID)项目的当地宇宙学的背景下,我们呈现了六个孤立的当地矮星系的详细的明星形成和化学浓缩历史。 LCID项目的主要目标之一是调查全球流程等宇宙的重生等的影响,或在矮星的演变中等内部机制等内部机制。我们展示了样本中的所有星系,包括那些非常早期结束星形形成的星系,例如DSPH和DLR / DSPH类型,在重新加化后形成了大部分恒星。这表明单独的食子化无法阻止它们中的星形形成,正如预期的那样。我们探讨了可能导致这些星系中明星形成的早期停止的替代机制。

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