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University of Cambridge > Talks.cam > Galaxies Discussion Group > Constraints on DM and the cusp/core problem with MUSE
Constraints on DM and the cusp/core problem with MUSEAdd to your list(s) Download to your calendar using vCal
If you have a question about this talk, please contact Sandro Tacchella. The concept of dark matter (DM) originates partly from the study of rotation curves in the 70s. Soon, shallow DM profiles (cores) were found in small galaxies instead of the steep (cusp) profiles expected from DM simulations. With the advancements in IFU technology and techniques, it is now possible to probe DM from the rotation curves of distant galaxies. We will show the current constraints on DM from MUSE surveys and discuss the prospects for the future. This talk is part of the Galaxies Discussion Group series. This talk is included in these lists:
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Other listsPhiliminality Cambridge Lucy Cavendish College public lecture series CU Pakistan SocietyOther talksDispersive models in biomechanics Lunch Public lecture: Unpackable Shapes and the Reinhardt Problem Machine Learning Sasakian and G2 Topology on Contact Calabi-Yau 7-manifolds Swarming rigid bodies: geometry and topology An introduction to the Langlands Program |
Nicolas Bouché (CNRS & CRAL)
Friday 22 September 2023, 11:30-12:30