| http://www.w3.org/ns/prov#value | - It might also form a basisfor comparison with future work.Within our formalism with a locally constant coolingtime, we find that (i) circular and eccentric discs alike cangravitationally fragment and form stars; (ii) the IMF offormed stars is a strong function of cooling time, becomingtop-heavy for marginally star-forming discs; (iii) star forma-tion feedback is indeed able to slow down disc fragm
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