The impact of environment and mergers on the H I content of galaxies in hydrodynamic simulations
>Magister Scientiae - MSc === We quantitatively examine the effects of merger and environment within a cosmological hydrodynamic simulation. We show that our simulation model broadly reproduces the observed scatter in H I at a given stellar mass as quantified by the HI mass function in bins of st...
Main Author: | Rafieferantsoa, Mika Harisetry |
---|---|
Other Authors: | Dave, Romeel |
Language: | en |
Published: |
University of the Western Cape
2016
|
Subjects: | |
Online Access: | http://hdl.handle.net/11394/4763 |
Similar Items
-
Neutral hydrogen in galaxies, its content and the effect of environment on its evolution
by: Rafieferantsoa, Mika Harisetry
Published: (2019) -
Formation & Evolution of early-types galaxies : Numerical simulations of galaxy mergers
by: Bois, Maxime
Published: (2011) -
The transformation of Spirals into S0 galaxies in the cluster environment
by: Mauro eD'onofrio, et al.
Published: (2015-08-01) -
Galaxy Populations in Massive Galaxy Clusters to z = 1.1: Color Distribution, Concentration, Halo Occupation Number and Red Sequence Fraction
by: Hennig, C., et al.
Published: (2017) -
Star formation rate and the assembly of galaxies in the early universe
by: Wang, Pin-Wei
Published: (2015)