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Autor:
Daniel Elsender, Matthew R. Bate
We present the analysis of the properties of large samples of protostellar discs formed in four radiation hydrodynamical simulations of star cluster formation. The four calculations have metallicities of 0.01, 0.1, 1 and 3 times solar metallicity. Th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d53bb054cff53b99b5f7d4a43f4ae670
