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- W2883007211 endingPage "1329" @default.
- W2883007211 startingPage "1304" @default.
- W2883007211 abstract "In order to better understand the relationship between feedback and galactic chemical evolution, we have developed a new model for stellar feedback at grid resolutions of only a few parsecs in global disk simulations, using the adaptive mesh refinement hydrodynamics code Enzo. For the first time in galaxy scale simulations, we simulate detailed stellar feedback from individual stars including asymptotic giant branch winds, photoelectric heating, Lyman-Werner radiation, ionizing radiation tracked through an adaptive ray-tracing radiative transfer method, and core collapse and Type Ia supernovae. We furthermore follow the star-by-star chemical yields using tracer fields for 15 metal species: C, N, O, Na, Mg, Si, S, Ca, Mn, Fe, Ni, As, Sr, Y, and Ba. We include the yields ejected in massive stellar winds, but greatly reduce the winds' velocities due to computational constraints. We describe these methods in detail in this work and present the first results from 500~Myr of evolution of an isolated dwarf galaxy with properties similar to a Local Group, low-mass dwarf galaxy. We demonstrate that our physics and feedback model is capable of producing a dwarf galaxy whose evolution is consistent with observations in both the Kennicutt-Schmidt relationship and extended Schmidt relationship. Effective feedback drives outflows with a greater metallicity than the ISM, leading to low metal retention fractions consistent with observations. Finally, we demonstrate that these simulations yield valuable information on the variation in mixing behavior of individual metal species within the multi-phase interstellar medium." @default.
- W2883007211 created "2018-08-03" @default.
- W2883007211 creator A5019489277 @default.
- W2883007211 creator A5078317510 @default.
- W2883007211 creator A5087474486 @default.
- W2883007211 date "2018-10-04" @default.
- W2883007211 modified "2023-10-17" @default.
- W2883007211 title "Simulating an isolated dwarf galaxy with multichannel feedback and chemical yields from individual stars" @default.
- W2883007211 cites W1488192889 @default.
- W2883007211 cites W1539883272 @default.
- W2883007211 cites W1624693442 @default.
- W2883007211 cites W1666700673 @default.
- W2883007211 cites W1766563480 @default.
- W2883007211 cites W1769129082 @default.
- W2883007211 cites W1831661775 @default.
- W2883007211 cites W1883916103 @default.
- W2883007211 cites W1910580027 @default.
- W2883007211 cites W1925826255 @default.
- W2883007211 cites W1963642624 @default.
- W2883007211 cites W1967433269 @default.
- W2883007211 cites W1969060985 @default.
- W2883007211 cites W1975019781 @default.
- W2883007211 cites W1977521416 @default.
- W2883007211 cites W1982706728 @default.
- W2883007211 cites W1983545063 @default.
- W2883007211 cites W1985063896 @default.
- W2883007211 cites W1987522415 @default.
- W2883007211 cites W1987635305 @default.
- W2883007211 cites W1993564394 @default.
- W2883007211 cites W1996116122 @default.
- W2883007211 cites W1999445914 @default.
- W2883007211 cites W2001068620 @default.
- W2883007211 cites W2005631644 @default.
- W2883007211 cites W2008429960 @default.
- W2883007211 cites W2011652587 @default.
- W2883007211 cites W2011868370 @default.
- W2883007211 cites W2014937117 @default.
- W2883007211 cites W2015295900 @default.
- W2883007211 cites W2020112982 @default.
- W2883007211 cites W2022645106 @default.
- W2883007211 cites W2026357841 @default.
- W2883007211 cites W2028896508 @default.
- W2883007211 cites W2031905411 @default.
- W2883007211 cites W2032365236 @default.
- W2883007211 cites W2033755233 @default.
- W2883007211 cites W2033950450 @default.
- W2883007211 cites W2034482962 @default.
- W2883007211 cites W2034933552 @default.
- W2883007211 cites W2038851723 @default.
- W2883007211 cites W2039789464 @default.
- W2883007211 cites W2040364743 @default.
- W2883007211 cites W2042081950 @default.
- W2883007211 cites W2043690401 @default.
- W2883007211 cites W2045028470 @default.
- W2883007211 cites W2046061553 @default.
- W2883007211 cites W2052624763 @default.
- W2883007211 cites W2054093933 @default.
- W2883007211 cites W2054403584 @default.
- W2883007211 cites W2054450804 @default.
- W2883007211 cites W2054801391 @default.
- W2883007211 cites W2055184402 @default.
- W2883007211 cites W2060277062 @default.
- W2883007211 cites W2063437365 @default.
- W2883007211 cites W2066398239 @default.
- W2883007211 cites W2067644575 @default.
- W2883007211 cites W2073207761 @default.
- W2883007211 cites W2073945818 @default.
- W2883007211 cites W2076246932 @default.
- W2883007211 cites W2077449384 @default.
- W2883007211 cites W2077678988 @default.
- W2883007211 cites W2079522592 @default.
- W2883007211 cites W2085926195 @default.
- W2883007211 cites W2088668851 @default.
- W2883007211 cites W2091055609 @default.
- W2883007211 cites W2099876653 @default.
- W2883007211 cites W2110349209 @default.
- W2883007211 cites W2113340703 @default.
- W2883007211 cites W2114246636 @default.
- W2883007211 cites W2119131940 @default.
- W2883007211 cites W2120027063 @default.
- W2883007211 cites W2125195055 @default.
- W2883007211 cites W2125939105 @default.
- W2883007211 cites W2126719454 @default.
- W2883007211 cites W2136336431 @default.
- W2883007211 cites W2138331350 @default.
- W2883007211 cites W2139466216 @default.
- W2883007211 cites W2140137154 @default.
- W2883007211 cites W2140888726 @default.
- W2883007211 cites W2148966198 @default.
- W2883007211 cites W2148972436 @default.
- W2883007211 cites W2151681625 @default.
- W2883007211 cites W2152856327 @default.
- W2883007211 cites W2153120512 @default.
- W2883007211 cites W2154213758 @default.
- W2883007211 cites W2156030349 @default.
- W2883007211 cites W2157378473 @default.
- W2883007211 cites W2159504674 @default.
- W2883007211 cites W2165003596 @default.