|COOKIES: By using this website you agree that we can place Google Analytics Cookies on your device for performance monitoring.|
The stellar IMF and the earliest phase of the assembly of the Milky Way
If you have a question about this talk, please contact mmg35.
The shape of the canonical IMF is briefly reviewed. Using the present day stellar populations in globular clusters as a constraint on their birth configurations these may be compared to observational data on star forming regions. Correlations appear, e.g. between the radius and the shape of the IMF versus the mass of the embedded cluster. Rather remarkable information is unearthed on the very earliest events that shaped the birth of the Milky Way galaxy.
This talk is part of the Institute of Astronomy Seminars series.
This talk is included in these lists:
Note that ex-directory lists are not shown.
Other listsBiological and Soft Systems Seminars Engineers Without Borders - Training British Antarctic Survey Happy Hour Seminar Series
Other talksFrom Graphon to Graphex: Models and Estimators for Sparse Networks using Exchangeable Random Measures tba Inhibition of phagocytosis by extracellular pathogens enteropathogenic and enterohaemorrhagic Escherichia coli Cambridge Rare Disease Network International Summit Wake effects in the ocean - from dolphins to CTDs via western boundary currents Unlocking the potential of synthetic biology to enhance human health