Globular clusters are among the oldest objects we know of, many likely to have formed at the epoch of reionization, and may have even contributed to it. Their formation, with their ubiquitous multiple stellar generations, remains an intriguing puzzle in astrophysics. Direct evidence indicates that they formed in a series of bursts, and each burst did not prevent the occurrence of the following ones, as if there was no negative feedback on star formation. Moreover, second-generation stars exhibit different light-element abundances, but no sign of enhancement by supernova products which, together with the lack of feedback, indicates that formation took place before supernovae started to affect the ISM. This suggests that, above a critical mass, stars fail to produce supernova events, but rather sink into black holes without ejecting much energy and heavy metals. This scenario of globular cluster formation has the attractive implication of suppressing star formation feedback for some ~10 million years, in practice leading to runaway star formation, analog to overcooling that in the absence of feedback would have turned most baryons into stars in the early Universe. Under such conditions, multiple episodes of star formation, incorporating stellar ejecta from previous bursts, appear to be unavoidable, thus accounting for the ubiquity of the multiple-generation phenomenon in globular clusters. If this is indeed the way globular clusters formed, then a generic ~10 Myr delayed feedback would have important implications for star formation in general, and in particular for the very high redshift Universe, helping to account for the unexpected frequency of bright/massive galaxies at z=9-16 revealed by JWST.
10/04/2024
Speaker: Alvio Renzini (INAF-Osservatorio Astronomico di Padova)
We are glad to invite you to the Rome Joint Astrophysics Colloquium (JAC), next April 10th at 14:30 CEST.
The Rome JAC is a joint initiative of the Physics Dept. of the Tor Vergata University of Rome, INAF - Astronomical Observatory of Rome, and INAF - Institute for Space Astrophysics and Planetology.
The talk will be held in a hybrid format allowing both virtual (through the link below) and in-person attendance (Aula Gratton, Astronomical Observatory of Rome).
Link for the remote connection: http://meet.google.com/zev-pdvv-gku