ALMA line survey maps eight converging filaments in Sgr B2(N) with 20-100 km/s/pc gradients and 0.16 M_sun/yr total accretion, indicating potential super stellar cluster formation via damp mergers of gas-rich cores.
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In Arp 147, collision-triggered star formation produced abundant young massive clusters whose mass function follows a Schechter shape with truncation at 6.2e5 solar masses, low disruption rate, and age-dependent formation efficiency.
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The Physical and chemical structure of Sagittarius B2 -- IV. Converging filaments in the high-mass cluster forming region Sgr B2(N)
ALMA line survey maps eight converging filaments in Sgr B2(N) with 20-100 km/s/pc gradients and 0.16 M_sun/yr total accretion, indicating potential super stellar cluster formation via damp mergers of gas-rich cores.
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Massive star clusters and clumps in the collisional ring galaxy Arp 147
In Arp 147, collision-triggered star formation produced abundant young massive clusters whose mass function follows a Schechter shape with truncation at 6.2e5 solar masses, low disruption rate, and age-dependent formation efficiency.