|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 listsThe Impact of Social Science Research Mathworks Institute of Astronomy Seminars
Other talksTBC (SP Workshop) Ethnic differences in mental health: does race matter? Epigenetics, Obesity and Metabolism Biobanking 2016 Intelligible Machine Learning Models for HealthCare OPUS - Keep track of your research data