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Core Mass Function in View of Fractal and Turbulent Filaments and Fibers
Indexado
WoS WOS:001428144500001
Scopus SCOPUS_ID:85218946301
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


Abstract



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.

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Disciplinas de Investigación



WOS
Astronomy & Astrophysics
Scopus
Astronomy And Astrophysics
Space And Planetary Science
SciELO
Sin Disciplinas

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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional



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Autores - Afiliación



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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Financiamiento



Fuente
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

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos



Agradecimiento
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.

Muestra la fuente de financiamiento declarada en la publicación.