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pro vyhledávání: '"Michael Kuffmeier"'
Autor:
Michael Kuffmeier
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 11 (2024)
The formation of protostars and their disks has been understood as the result of the gravitational collapse phase of an accumulation of dense gas that determines the mass reservoir of the star-disk system. Against this background, the broadly applied
Externí odkaz:
https://doaj.org/article/c0e5862d2459478ab609dd2308873afb
Publikováno v:
Kuffmeier, M, Jensen, S S & Haugbolle, T 2023, ' Rejuvenating infall : a crucial yet overlooked source of mass and angular momentum ', European Physical Journal Plus, vol. 138, no. 3, 272 . https://doi.org/10.1140/epjp/s13360-023-03880-y
MHD models and the observation of accretion streamers confirmed that protostars can undergo late accretion events after the initial collapse phase. To provide better constraints, we study the evolution of stellar masses in MHD simulations of a (4 pc)
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c1d02ae6f71eafb93d3b7c85cbf95c32
Publikováno v:
Astrophysical Journal; 9/1/2017, Vol. 846 Issue 1, p1-1, 1p
Autor:
Michael Kuffmeier, Troels Frostholm Mogensen, Troels Haugbølle, Martin Bizzarro, Åke Nordlund
Publikováno v:
Astrophysical Journal; 7/20/2016, Vol. 826 Issue 1, p1-1, 1p