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| zotero(3)(+0000000): LibreOfficePlugin: Read 3 [[0,1],["ITEM CSL_CITATION {\"citationID\":\"zVFGsF7E\",\"properties\":{\"formattedCitation\":\"(ADAMS, 2003; Buie II et al., 2020)\",\"plainCitation\":\"(ADAMS, 2003; Buie II et al., 2020)\",\"noteIndex\":0},\"citationItems\":[{\"id\":28,\"uris\":[\"http://zotero.org/users/23863/items/U8FETR9Y\"],\"uri\":[\"http://zotero.org/users/23863/items/U8FETR9Y\"],\"itemData\":{\"id\":28,\"type\":\"chapter\",\"abstract\":\"Another dimension of the institutional neutrality debate revolves around admissions. Who shall be allowed to go to college? What kind of college? How are the applicant’s credentials to be judged? Shall such extraneous variables as race be given any consideration? Is it proper for universities to set quotas to accommodate minorities, or go even further to a policy of “open admissions”?\\nAgain, the debate basically turns on the conception of the university, and the role it plays in society. To the “classicist,” the university has three primary obligations: first, a commitment to transmit high culture—to shape students’ mind and\",\"container-title\":\"The Test\",\"ISBN\":\"978-0-87013-648-1\",\"page\":\"183-202\",\"publisher\":\"Michigan State University Press\",\"source\":\"JSTOR\",\"title\":\"THE GUARDIANS OF EXCELLENCE\",\"URL\":\"http://www.jstor.org/stable/10.14321/j.ctt130hjnp.11\",\"editor\":[{\"family\":\"ADAMS\",\"given\":\"WALTER\"}],\"accessed\":{\"date-parts\":[[\"2017\",7,20]]},\"issued\":{\"date-parts\":[[\"2003\"]]}}},{\"id\":791,\"uris\":[\"http://zotero.org/users/23863/items/AIYNF6FN\"],\"uri\":[\"http://zotero.org/users/23863/items/AIYNF6FN\"],\"itemData\":{\"id\":791,\"type\":\"article-journal\",\"abstract\":\"The circumgalactic medium (CGM) of nearby star-forming galaxies shows clear indications of OVI absorption accompanied by little to no detectable NV absorption. This unusual spectral signature, accompanied by highly non-uniform absorption from lower ionization state species, indicates that the CGM must be viewed as a dynamic, multiphase medium, such as occurs in the presence of turbulence. Motivated by previous isotropic turbulent simulations, we carry out chemodynamical simulations of stratified media in a Navarro-Frenk-White (NFW) gravitational potential with a total mass of $10^{12}$ solar masses and turbulence that decreases radially. The simulations assume a metallicity of 0.3 solar, a redshift zero metagalatic UV background, and they track ionizations, recombinations, and species-by-species radiative cooling using the MAIHEM package. We compare a suite of ionic column densities with the COS-Halos sample of low-redshift star-forming galaxies. Turbulence with an average one-dimensional velocity dispersion approximately 40 km/s, corresponding to an energy injection rate of approximately $10^{49}$ erg/yr, produces a CGM that matches many of the observed ionic column densities and ratios. In this simulation, the NVI to OVI ratio is suppressed from its equilibrium value due to a combination of radiative cooling and cooling from turbulent mixing. This level of turbulence is consistent with expectations from observations of better constrained, higher-mass systems, and could be sustained by energy input from supernovae, gas inflows, and dynamical friction from dark matter subhalos. We also conduct a higher resolution run which yields smaller-scale structures, but remains in agreement with observations.\",\"container-title\":\"arXiv:2006.03066 [astro-ph]\",\"note\":\"arXiv: 2006.03066\",\"source\":\"arXiv.org\",\"title\":\"Modeling Photoionized Turbulent Material in the Circumgalactic Medium II: Effect of Turbulence within a Stratified Medium\",\"title-short\":\"Modeling Photoionized Turbulent Material in the Circumgalactic Medium II\",\"URL\":\"http://arxiv.org/abs/2006.03066\",\"author\":[{\"family\":\"Buie II\",\"given\":\"Edward\"},{\"family\":\"Gray\",\"given\":\"William J.\"},{\"family\":\"Scannapieco\",\"given\":\"Evan\"},{\"family\":\"Safarzadeh\",\"given\":\"Mohammadtaher\"}],\"accessed\":{\"date-parts\":[[\"2020\",6,8]]},\"issued\":{\"date-parts\":[[\"2020\",6,4]]}}}],\"schema\":\"https://github.com/citation-style-language/schema/raw/master/csl-citation.json\"}","BIBL {\"uncited\":[],\"omitted\":[],\"custom\":[[[\"http://zotero.org/users/23863/items/AIYNF6FN\"],\"Buie II, E., Gray, W. J., Scannapieco, E., & Safarzadeh, M. (2020). Modeling Photoionizeasgdasdgasdgd Turbulent Material in the Circumgalactic Medium II: Effect of Turbulence within a Stratified Medium. {\\\\i{}ArXiv:2006.03066 [Astro-Ph]}. http://arxiv.org/abs/2006.03066\"]]} CSL_BIBLIOGRAPHY"],[0,0]] | |
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