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We use the APOSTLE suite of cosmological simulations to examine the role of the cosmic ionizing background in regulating star formation (SF) in low-mass LCDM halos. In agreement with earlier work, we find that, after reionization, SF can only proceed
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8c812c275a53fabbcba4f2f518470674
