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| DOI | 10.1088/1674-4527/ADB15A | ||||
| Año | 2025 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
We propose that the core mass function (CMF) can be driven by filament fragmentation. To model a star-forming system of filaments and fibers, we develop a fractal and turbulent tree with a fractal dimension of 2 and a Larson's law exponent (beta) of 0.5. The fragmentation driven by convergent flows along the splines of the fractal tree yields a Kroupa-IMF-like CMF that can be divided into three power-law segments with exponents alpha = -0.5, -1.5, and -2, respectively. The turnover masses of the derived CMF are approximately four times those of the Kroupa IMF, corresponding to a star formation efficiency of 0.25. Adopting beta = 1/3, which leads to fractional Brownian motion along the filament, may explain a steeper CMF at the high-mass end, with alpha = -3.33 close to that of the Salpeter IMF. We suggest that the fibers of the tree are basic building blocks of star formation, with similar properties across different clouds, establishing a common density threshold for star formation and leading to a universal CMF.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Liu, Xunchuan | - |
CASSACA - China
Leiden Univ - Países Bajos Chinese Academy of Sciences - China Sterrewacht Leiden - Países Bajos |
| 2 | Liu, Tie | - |
CASSACA - China
Chinese Academy of Sciences - China |
| 3 | Mai, Xiaofeng | - |
CASSACA - China
Univ Helsinki - Finlandia Chinese Academy of Sciences - China Helsingin Yliopisto - Finlandia |
| 4 | Cheng, Yu | - |
Natl Astron Observ Japan - Japón
National Institutes of Natural Sciences - National Astronomical Observatory of Japan - Japón |
| 5 | Jiao, Sihan | - |
CASSACA - China
National Astronomical Observatories Chinese Academy of Sciences - China Chinese Academy of Sciences - China |
| 6 | Jiao, Wenyu | - |
CASSACA - China
Chinese Academy of Sciences - China |
| 7 | Liu, Hongli | - |
Yunnan Univ - China
Yunnan University - China |
| 8 | Zhang, Siju | - |
Universidad de Chile - Chile
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| Fuente |
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| National Natural Science Foundation of China |
| National Key R&D Program of China |
| National Key Research and Development Program of China |
| Chinese Academy of Sciences |
| National Natural Science Foundation of China (NSFC) |
| Strategic Priority Research Program of the Chinese Academy of Sciences |
| Agradecimiento |
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| X.L. acknowledges the support of the Strategic Priority Research Program of the Chinese Academy of Sciences under grant No. XDB0800303, the National Key R&D Program of China under grant No. 2022YFA1603100, and the National Natural Science Foundation of China (NSFC, Grant No. 12203086). We also thank the anonymous referee for the insightful comments, which helped refine this work. |
| X.L. acknowledges the support of the Strategic Priority Research Program of the Chinese Academy of Sciences under grant No. XDB0800303, the National Key R&D Program of China under grant No. 2022YFA1603100, and the National Natural Science Foundation of China (NSFC, Grant No. 12203086). We also thank the anonymous referee for the insightful comments, which helped refine this work. |