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- W4315929334 abstract "We present a statistical study of a sample of 17 hub-filament-system (HFS) clouds of high-mass star formation using high-angular resolution ($sim$1-2 arcsecond) ALMA 1.3mm and 3mm continuum data. The sample includes 8 infrared (IR)-dark and 9 IR-bright types, which correspond to an evolutionary sequence from the IR-dark to IR-bright stage. The central massive clumps and their associated most massive cores are observed to follow a trend of increasing mass ($M$) and mass surface density ($Sigma$) with evolution from IR-dark to IR-bright stage. In addition, a mass-segregated cluster of young stellar objects (YSOs) are revealed in both IR-dark and IR-bright HFSs with massive YSOs located in the hub and the population of low-mass YSOs distributed over larger areas. Moreover, outflow feedback in all HFSs are found to escape preferentially through the inter-filamentary diffuse cavities, suggesting that outflows would render a limited effect on the disruption of the HFSs and ongoing high-mass star formation therein. From the above observations, we suggest that high-mass star formation in the HFSs can be described by a multi-scale mass accretion/transfer scenario, from hub-composing filaments through clumps down to cores, that can naturally lead to a mass-segregated cluster of stars." @default.
- W4315929334 created "2023-01-14" @default.
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- W4315929334 date "2023-01-13" @default.
- W4315929334 modified "2023-10-15" @default.
- W4315929334 title "Evidence of high-mass star formation through multiscale mass accretion in hub-filament-system clouds" @default.
- W4315929334 cites W1562778997 @default.
- W4315929334 cites W1964867136 @default.
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- W4315929334 cites W2013965924 @default.
- W4315929334 cites W2027217802 @default.
- W4315929334 cites W2042169845 @default.
- W4315929334 cites W2054720561 @default.
- W4315929334 cites W2057600434 @default.
- W4315929334 cites W2073961934 @default.
- W4315929334 cites W2077638261 @default.
- W4315929334 cites W2080022127 @default.
- W4315929334 cites W2092575992 @default.
- W4315929334 cites W2149823722 @default.
- W4315929334 cites W2156271110 @default.
- W4315929334 cites W2156658280 @default.
- W4315929334 cites W2200634234 @default.
- W4315929334 cites W2228723868 @default.
- W4315929334 cites W2290856567 @default.
- W4315929334 cites W2562597233 @default.
- W4315929334 cites W2610689502 @default.
- W4315929334 cites W2740803923 @default.
- W4315929334 cites W2784373895 @default.
- W4315929334 cites W2798908258 @default.
- W4315929334 cites W2886860723 @default.
- W4315929334 cites W2888532099 @default.
- W4315929334 cites W2911358814 @default.
- W4315929334 cites W2921038094 @default.
- W4315929334 cites W2925297590 @default.
- W4315929334 cites W2953590102 @default.
- W4315929334 cites W2963102747 @default.
- W4315929334 cites W2964598364 @default.
- W4315929334 cites W2974309548 @default.
- W4315929334 cites W3012978202 @default.
- W4315929334 cites W3026718024 @default.
- W4315929334 cites W3033465016 @default.
- W4315929334 cites W3039155106 @default.
- W4315929334 cites W3046800483 @default.
- W4315929334 cites W3086230335 @default.
- W4315929334 cites W3094220782 @default.
- W4315929334 cites W3098876014 @default.
- W4315929334 cites W3099123091 @default.
- W4315929334 cites W3099889244 @default.
- W4315929334 cites W3100193471 @default.
- W4315929334 cites W3100213073 @default.
- W4315929334 cites W3100911696 @default.
- W4315929334 cites W3101145158 @default.
- W4315929334 cites W3101710491 @default.
- W4315929334 cites W3101864204 @default.
- W4315929334 cites W3102967193 @default.
- W4315929334 cites W3103692774 @default.
- W4315929334 cites W3103708103 @default.
- W4315929334 cites W3104199804 @default.
- W4315929334 cites W3104423841 @default.
- W4315929334 cites W3104764529 @default.
- W4315929334 cites W3105041955 @default.
- W4315929334 cites W3105719588 @default.
- W4315929334 cites W3106320302 @default.
- W4315929334 cites W3107966079 @default.
- W4315929334 cites W3112631224 @default.
- W4315929334 cites W3124073635 @default.