Boundary Conditions in Hydrodynamic Simulations of Isolated Galaxies and Their Impact on the Gas-loss Processes

Autor: Anderson Caproni, Gustavo A. Lanfranchi, Amâncio C. S. Friaça, Jennifer F. Soares

Publikováno v: The Astrophysical Journal, Vol 944, Iss 1, p 11 (2023)

Three-dimensional hydrodynamic simulations are commonly used to study the evolution of the gaseous content in isolated galaxies, besides its connection with galactic star formation histories. Stellar winds, supernova blasts, and black hole feedback a

Externí odkaz: https://doaj.org/article/9a1b32e6fbda4cdebade493dc2b0fea2

The S2 Stream: the shreds of a primitive dwarf galaxy

Autor: Sergey E. Koposov, Camila Navarrete, Carlos Allende Prieto, Luca Sbordone, Zhen Yuan, Luis Peralta de Arriba, David Aguado, Jonay I. González Hernández, Vasily Belokurov, Gustavo A. Lanfranchi, Matthew Shetrone, Francesca Matteucci, N. Wyn Evans, Julio Chanamé, G. C. Myeong

Publikováno v: Aguado, D S, Myeong, G C, Belokurov, V, Evans, N W, Koposov, S E, Prieto, C A, Lanfranchi, G A, Matteucci, F, Shetrone, M, Sbordone, L, Navarrete, C, Hernández, J I G, Chanamé, J, Arriba, L P D & Yuan, Z 2021, ' The S2 Stream : the shreds of a primitive dwarf galaxy ', Monthly Notices of the Royal Astronomical Society, vol. 500, no. 1, pp. 889-910 . https://doi.org/10.1093/mnras/staa3250

The S2 stream is a kinematically cold stream that is plunging downwards through the Galactic disc. It may be part of a hotter and more diffuse structure called the Helmi stream. We present a multi-instrument chemical analysis of the stars in the meta

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5cc2f7f7c451d4181541bcae31ce079a

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

Autor: Gustavo A. Lanfranchi, Diego Falceta-Gonçalves, Anderson Caproni, Grzegorz Kowal, Gabriel Henrique Campos Baião

Publikováno v: Proceedings of the International Astronomical Union. 14:49-52

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

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::9ead2ad4aa1ace0e4aac5c5d3fda5ea2
https://doi.org/10.1017/s1743921318006695

The gas-loss evolution in dwarf spheroidal galaxies: Supernova feedback and environment effects in the case of the local group galaxy Ursa Minor

Autor: Gustavo A. Lanfranchi, Anderson Caproni

Publikováno v: Proceedings of the International Astronomical Union. 15:117-118

In this work, we performed two distinct non-cosmological, three-dimensional hydrodynamic simulations that evolved the gas component of a galaxy similar to the classical dwarf spheroidal galaxy Ursa Minor. Both simulations take into account types II a

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::a7fd55e85276805ff46a547b869eb267
https://doi.org/10.1017/s1743921320002161

The mass-loss process in dwarf galaxies from 3D hydrodynamical simulations: the role of dark matter and starbursts

Autor: L. O. Ruiz, Anderson Caproni, Gustavo A. Lanfranchi, Diego Falceta-Gonçalves

Publikováno v: Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP

Theoretical $\Lambda$CDM cosmological models predict a much larger number of low mass dark matter haloes than has been observed in the Local Group of galaxies. One possible explanation is the increased difficulty of detecting these haloes if most of

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7dc8b57361902fca7823ef34e51d30ce
https://doi.org/10.1093/mnras/sts425