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• W2883983485 abstract "From studying the cosmic microwave background, we know our Universe started out very simple. It was by and large homogeneous and isotropic, with small fluctuations that can be described by linear perturbation theory. In stark contrast, the Universe today is highly structured on a vast range of length and mass scales. In the evolution towards increasing complexity, the formation of the first stars marks a primary transition event. The first generation of stars, the so-called Population III (or Pop. III) build up from truly metal-free primordial gas. They have long been thought to live short, solitary lives, with only one massive star forming per halo. However, in recent years this simple picture has undergone substantial revision, and we now understand that stellar birth in the early Universe is subject to the same complexity as star formation at present days. In this chapter, I review the current state of the field. I begin by introducing the basics concepts of star-formation theory and by discussing the typical environment in which Pop. III stars are thought to form. Then I argue that the accretion disk that builds up in the center of a halo is likely to fragment, resulting in the formation of a cluster of stars with a wide range of masses, and I speculate about how this process may be influenced by stellar feedback, the presence of magnetic fields, the energy input from dark matter annihilation, and the occurrence of large- scale streaming velocities between baryons and dark matter. Finally, I discuss direct and indirect constraints on Pop. III star formation from high-redshift observations and from the search for extremely metal-poor stars in the Milky Way and its satellites." @default.
• W2883983485 created "2018-08-03" @default.
• W2883983485 creator A5062809181 @default.
• W2883983485 date "2019-04-28" @default.
• W2883983485 modified "2023-10-12" @default.
• W2883983485 title "Formation of the first stars" @default.
• W2883983485 cites W1552965972 @default.
• W2883983485 cites W1584089510 @default.
• W2883983485 cites W1639285581 @default.
• W2883983485 cites W1672824258 @default.
• W2883983485 cites W1809134323 @default.
• W2883983485 cites W1828861430 @default.
• W2883983485 cites W1837696333 @default.
• W2883983485 cites W1861231237 @default.
• W2883983485 cites W1861753695 @default.
• W2883983485 cites W1965713361 @default.
• W2883983485 cites W1973764912 @default.
• W2883983485 cites W1974857090 @default.
• W2883983485 cites W1975627161 @default.
• W2883983485 cites W1975889887 @default.
• W2883983485 cites W1976255534 @default.
• W2883983485 cites W1981638202 @default.
• W2883983485 cites W1983471014 @default.
• W2883983485 cites W1987475110 @default.
• W2883983485 cites W1989528790 @default.
• W2883983485 cites W1990386756 @default.
• W2883983485 cites W1998581888 @default.
• W2883983485 cites W2003407741 @default.
• W2883983485 cites W2006747435 @default.
• W2883983485 cites W2008065079 @default.
• W2883983485 cites W2012927551 @default.
• W2883983485 cites W2012997244 @default.
• W2883983485 cites W2018627919 @default.
• W2883983485 cites W2019428480 @default.
• W2883983485 cites W2020575263 @default.
• W2883983485 cites W2022645106 @default.
• W2883983485 cites W2023001659 @default.
• W2883983485 cites W2027334559 @default.
• W2883983485 cites W2027544184 @default.
• W2883983485 cites W2029077494 @default.
• W2883983485 cites W2030191206 @default.
• W2883983485 cites W2030489439 @default.
• W2883983485 cites W2030644355 @default.
• W2883983485 cites W2031117379 @default.
• W2883983485 cites W2031669070 @default.
• W2883983485 cites W2031768088 @default.
• W2883983485 cites W2034649301 @default.
• W2883983485 cites W2035547408 @default.
• W2883983485 cites W2036179433 @default.
• W2883983485 cites W2036447390 @default.
• W2883983485 cites W2040912209 @default.
• W2883983485 cites W2041584190 @default.
• W2883983485 cites W2041893863 @default.
• W2883983485 cites W2044688893 @default.
• W2883983485 cites W2044919768 @default.
• W2883983485 cites W2048047963 @default.
• W2883983485 cites W2050354875 @default.
• W2883983485 cites W2051431923 @default.
• W2883983485 cites W2051762527 @default.
• W2883983485 cites W2052528558 @default.
• W2883983485 cites W2061094501 @default.
• W2883983485 cites W2062280374 @default.
• W2883983485 cites W2062719264 @default.
• W2883983485 cites W2067827212 @default.
• W2883983485 cites W2068531270 @default.
• W2883983485 cites W2068939329 @default.
• W2883983485 cites W2073092864 @default.
• W2883983485 cites W2077678988 @default.
• W2883983485 cites W2078484744 @default.
• W2883983485 cites W2080886544 @default.
• W2883983485 cites W2083870045 @default.
• W2883983485 cites W2083950714 @default.
• W2883983485 cites W2085125001 @default.
• W2883983485 cites W2085926195 @default.
• W2883983485 cites W2088514135 @default.
• W2883983485 cites W2089177363 @default.
• W2883983485 cites W2096896195 @default.
• W2883983485 cites W2097068720 @default.
• W2883983485 cites W2100183643 @default.
• W2883983485 cites W2100758318 @default.
• W2883983485 cites W2100973451 @default.
• W2883983485 cites W2102639000 @default.
• W2883983485 cites W2104311895 @default.
• W2883983485 cites W2106404450 @default.
• W2883983485 cites W2108264928 @default.
• W2883983485 cites W2108635461 @default.
• W2883983485 cites W2114382268 @default.
• W2883983485 cites W2129495060 @default.
• W2883983485 cites W2137885638 @default.
• W2883983485 cites W2137906322 @default.
• W2883983485 cites W2140347367 @default.
• W2883983485 cites W2140473010 @default.
• W2883983485 cites W2141156813 @default.
• W2883983485 cites W2141687171 @default.
• W2883983485 cites W2148047497 @default.
• W2883983485 cites W2153220281 @default.
• W2883983485 cites W2160547773 @default.
• W2883983485 cites W2171351131 @default.

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