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pro vyhledávání: '"Jaffa, Sarah E."'
The conditions required for massive star formation are debated, particularly whether massive stars must form in conjunction with massive clusters. Some authors have advanced the view that stars of any mass (below the total cluster mass) can form in c
Externí odkaz:
http://arxiv.org/abs/2309.05635
The interstellar medium is highly structured, presenting a range of morphologies across spatial scales. The large data sets resulting from observational surveys and state-of-the-art simulations studying these hierarchical structures means that identi
Externí odkaz:
http://arxiv.org/abs/2208.07509
Star clusters are known to be formed in turbulent molecular clouds. How turbulence is driven in molecular clouds and what effect this has on star formation is still unclear. We compare a simulation setup with turbulent driving everywhere in a periodi
Externí odkaz:
http://arxiv.org/abs/2208.05474
Publikováno v:
Monthly Notices of the Royal Astronomical Society; 11/15/2023, Vol. 525 Issue 4, p6182-6190, 9p
Akademický článek
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Publikováno v:
Monthly Notices of the Royal Astronomical Society; Nov2022, Vol. 516 Issue 3, p4212-4219, 8p
Akademický článek
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Autor:
Francesco Strafella, Stefano Pezzuto, Nicola Schneider, Sergio Molinari, Davide Elia, S. E. Jaffa, Eugenio Schisano, Patrick Hennebelle, Sami Dib
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2018, 481 (1), pp.509-532. ⟨10.1093/mnras/sty2170⟩
Monthly Notices of the Royal Astronomical Society, 2018, 481 (1), pp.509-532. ⟨10.1093/mnras/sty2170⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2018, 481 (1), pp.509-532. ⟨10.1093/mnras/sty2170⟩
Monthly Notices of the Royal Astronomical Society, 2018, 481 (1), pp.509-532. ⟨10.1093/mnras/sty2170⟩
The multifractal geometry remains an under-exploited approach to describe and quantify the large-scale structure of interstellar clouds. In this paper, the typical tools of multifractal analysis are applied to Herschel far-infrared (70-500 $\mu$m) du
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::913dec501b73412c073d1d73859d4990
https://academic.oup.com/mnras/issue
https://academic.oup.com/mnras/issue