COOKIES: By using this website you agree that we can place Google Analytics Cookies on your device for performance monitoring. |
University of Cambridge > Talks.cam > Galaxies Discussion Group > Galaxy kinematics within the cosmic web
Galaxy kinematics within the cosmic webAdd to your list(s) Download to your calendar using vCal
If you have a question about this talk, please contact Sandro Tacchella. The study of the interplay between galaxy angular momentum and structures in the cosmic web is a powerful tool to constrain galaxy evolution scenarios. Taking advantage of the Integral Field Spectroscopic SAMI galaxy survey and the GAMA redshift survey, I will present measurements of the kinematic alignments of the galaxies’ spin axes with respect to nearby cosmic filaments as a function of various galaxy properties. The mass of the bulge is the primary parameter in determining these spin-filament alignment. I will discuss these findings in comparison to secular star formation quenching and in terms of possible evolution pathways for galaxies. This talk is part of the Galaxies Discussion Group series. This talk is included in these lists:
Note that ex-directory lists are not shown. |
Other listsICE Research Seminar Series Diversity Cinema at UIS criOther talksIntroduction to Light Microscopy Artificial Intelligence in Cancer A robust and scalable approach to Bayesian doubly-intractable problems Unsteady aerodynamics in large-disturbance flows: Gust encounters and maneuvering wings |