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 > The structure of the interstellar medium as probe of the baryonic physics of galaxy evolution
The structure of the interstellar medium as probe of the baryonic physics of galaxy evolutionAdd to your list(s) Download to your calendar using vCal
If you have a question about this talk, please contact Sandro Tacchella. Understanding what shapes the cold gas component of galaxies is crucial to our understanding of galaxy evolution. Not only because cold gas provides the fuel for star formation, but also because its structural and kinematic properties are affected by the resultant stellar feedback. I will present detailed analysis of isolated galaxy and cosmological simulations and discuss how the interstellar medium (and star formation) are affected by the gravitational potential of galaxies, as well as how the interstellar medium structure can be a probe for different star formation and feedback models. 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 listsFeminism CamBRAIN talks EED Film Series: 'City of God'Other talksAveraging to Higher Depth Mock Modular Forms Reviewing Early Rome Through New Approaches Modelling airborne viral transmission in enclosed settings and comparing mitigations Vehicle-bridge interaction in railways: forward and inverse applications Communicating Maths and Stats is Just Like all Other Communication (Except When it Isn’t) |