{"paper":{"title":"A Global Model For Circumgalactic and Cluster-Core Precipitation","arxiv_id":"1607.02212","primary_cat":"astro-ph.GA","submitted_at":"2016-07-08T02:23:46+00:00","version_compiled":"v3"},"notice":"Every quoted sentence is the authors' text from the arXiv listing abstract. Labels and probabilities are the outputs of classifier-1.13.0 on the question bank abstract-p1-20260923, exactly as returned. 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stationary medium in which thermal balance is explicitly maintained.","hedge":{"p":0.67,"label":"asserted"},"own_p":0.59,"main_claim_p":0.02,"quantitative":true,"quantitative_p":0.51,"role_probabilities":{"gap":0.0,"method":0.88,"result":0.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.12,"interpretation":0.0}},{"i":2,"p":0.61,"id":"s2","own":true,"role":"method","text":"Analytic exploration of these two modes provides insights into the relationships between the local ratio of the cooling and freefall time scales (i.e., t_cool / t_ff), the large-scale gradient of specific entropy, and development of precipitation and multiphase media in circumgalactic gas.","hedge":{"p":0.8,"label":"asserted"},"own_p":0.88,"main_claim_p":0.05,"quantitative":false,"quantitative_p":0.37,"role_probabilities":{"gap":0.0,"method":0.61,"result":0.01,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.31,"interpretation":0.07}},{"i":3,"p":0.69,"id":"s3","own":true,"role":"method","text":"We then use these analytic findings to interpret recent simulations of circumgalactic gas in which global thermal balance is maintained.","hedge":{"p":0.89,"label":"asserted"},"own_p":0.82,"main_claim_p":0.04,"quantitative":false,"quantitative_p":0.06,"role_probabilities":{"gap":0.0,"method":0.69,"result":0.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.26,"interpretation":0.05}},{"i":4,"p":0.97,"id":"s4","own":true,"role":"result","text":"We show that long-lasting configurations of gas with 5 < t_cool / t_ff < 20 and radial entropy profiles similar to observations of local cool-core galaxy cluster cores are a natural outcome of precipitation-regulated feedback.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.9,"main_claim_p":0.74,"quantitative":true,"quantitative_p":0.99,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.97,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.0,"interpretation":0.03}},{"i":5,"p":0.5,"id":"s5","own":true,"role":"future_work","text":"We conclude with some observational predictions that follow from these models.","hedge":{"p":0.68,"label":"unclear"},"own_p":0.61,"main_claim_p":0.04,"quantitative":false,"quantitative_p":0.03,"role_probabilities":{"gap":0.0,"method":0.01,"result":0.01,"background":0.0,"limitation":0.0,"future_work":0.5,"contribution":0.46,"interpretation":0.02}},{"i":6,"p":0.96,"id":"s6","own":false,"role":"limitation","text":"This work focuses primarily on precipitation and AGN feedback in galaxy cluster cores, because that is where the observations of multiphase gas around galaxies are most 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