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The hydrodynamic evolution of the gas content in the dSph galaxy Ursa Minor induced by the feedback from types Ia and II supernovae

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Author(s):
Caproni, Anderson ; Lanfranchi, Gustavo A. ; Campos Baiao, Gabriel H. ; Kowal, Grzegorz ; Falceta-Goncalves, Diego ; McQuinn, KBW ; Stierwalt, S
Total Authors: 7
Document type: Journal article
Source: DWARF GALAXIES: FROM THE DEEP UNIVERSE TO THE PRESENT; v. 14, n. S344, p. 4-pg., 2019-01-01.
Abstract

Dwarf spheroidal galaxies of the Local Group share a similar characteristic nowadays: a low amount of gas in their interiors. In this work, we present results from a three-dimensional hydrodynamical simulation of the gas inside an object with similar characteristics of the Ursa Minor galaxy. We evolved the initial gas distribution over 3 Gyr, considering the effects of the types Ia and II supernovae. The instantaneous supernovae rates were derived from a chemical evolution model applied to spectroscopic data of the Ursa Minor galaxy. Our simulation shows that the amount of gas that is lost varies with time and galactocentric radius. The highest gas-loss rates occurred during the first 600 Myr of evolution. Our results also indicate that types Ia and II supernovae must be essential drivers of the gas loss in Ursa Minor galaxy (and probably in other similar dwarf galaxies). (AU)

FAPESP's process: 14/11156-4 - What drives the stellar mass growth of Early-Type galaxies? Born or made: the saga continues
Grantee:Reinaldo Ramos de Carvalho
Support Opportunities: Research Projects - Thematic Grants
FAPESP's process: 17/25651-5 - Numerical studies of extragalactic objects in the local universe and at high redshifts
Grantee:Anderson Caproni
Support Opportunities: Regular Research Grants
FAPESP's process: 17/03173-4 - Gas removal in the Ursa Minor galaxy: linking hydrodynamics and chemical evolution models
Grantee:Anderson Caproni
Support Opportunities: Regular Research Grants - Publications - Scientific article
FAPESP's process: 09/54006-4 - A computer cluster for the Astronomy Department of the University of São Paulo Institute of Astronomy, Geophysics and Atmospheric Sciences and for the Cruzeiro do Sul University Astrophysics Center
Grantee:Elisabete Maria de Gouveia Dal Pino
Support Opportunities: Multi-user Equipment Program