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pro vyhledávání: '"Yelverton, BM"'
Autor:
Kennedy, GM, Matrà, L, Facchini, S, Milli, J, Panić, O, Price, D, Wilner, DJ, Wyatt, MC, Yelverton, BM
Nearly all young stars are initially surrounded by ‘protoplanetary’ disks of gas and dust, and in the case of single stars at least 30% of these disks go on to form planets1. The process of protoplanetary disk formation can result in initial misa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=core_ac_uk__::dc7afc281b8ae583eff29ff9aa0bec8b
https://eprints.whiterose.ac.uk/154449/1/1901.05018.pdf
https://eprints.whiterose.ac.uk/154449/1/1901.05018.pdf
