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.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.GA 1years
2026 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
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.