The supernova remnant population of the Small Magellanic Cloud

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Fig. 2

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P × V^1∕2 of SNRs in SMC (orange triangles, this work) and LMC (grey plus signs, MHK16) as a function of their size. Lines of constant SN energy (times filling factor f, see text in Sect. 4.3.1) are overplotted in units of 10⁵¹ erg ≡1 foe.

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