Probing the dawn of galaxies: star formation and feedback in the JWST era through the GAEA model
Astronomy & AstrophysicsThe James Webb Space Telecope opened a new window for the study of the highest redshift (z > 7) Universe. This work presents a theoretical investigation of the very high-redshift Universe using the state-of-the-art GALaxy Evolution and Assembly (GAEA ...
Cantarella Sebastiano +6 more
doaj +1 more source
Galáxias post-starburst no universo local [PDF]
, 2014 Dissertação (mestrado) - Universidade Federal de Santa Catarina, Centro de Ciências Físicas e Matemáticas, Programa de Pós-Graduação em Física, Florianópolis, 2014Galáxias post-starburst (PSB) apresentam espectros com fortes linhas de absorção na série ...
Werle, Ariel
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The Role of Stellar Feedback in Galaxy Evolution
, 2009 Aiming at understanding the role of stellar feedback in galaxy evolution, I present a study of the hot interstellar medium in several representative galaxies, based primarily on X-ray observations as well as theoretical modelling. I find that, in the massive disk galaxies NGC2613 and M104, the observed amount of hot gas is much less than that ...
openaire +3 more sources
The importance of radiative feedback for the stellar initial mass function [PDF]
Monthly Notices of the Royal Astronomical Society, 2009 Published in MNRAS, 18 pages, 11 figures.
openaire +3 more sources
cx2204/stellar-radius: stellar radius microphysics
, 2022 Full Changelog: https://github.com/cx2204/stellar-radius/commits/v1.
cx2204
core +1 more source
Validating the CROCODILE Model Within the AGORA Galaxy Simulation Framework
GalaxiesNumerical galaxy formation simulations are sensitive to numerical methods and sub-grid physics models, making code comparison projects essential for quantifying uncertainties.
Pablo Granizo +2 more
doaj +1 more source
Searching for Stellar-feedback-driven Outflow Signatures: A Deep Dive into NGC 3741
The Astrophysical JournalStellar feedback drives winds and outflows critical to the baryon cycles of low-mass galaxies whose shallow gravitational potential wells make them particularly susceptible to mass and metal loss through outflows. However, spatially resolved observations
Lexi N. Gault +7 more
doaj +1 more source
Bursty Star Formation in Dwarfs is Sensitive to Numerical Choices in Supernova Feedback Models
The Astrophysical JournalSimulations of galaxy formation are mostly unable to resolve the energy-conserving phase of individual supernova events, having to resort to subgrid models to distribute the energy and momentum resulting from stellar feedback.
Eric Zhang +8 more
doaj +1 more source
Homogeneous spectroscopic parameters for bright planet host stars from the northern hemisphere. The impact on stellar and planetary mass [PDF]
, 2015 This work is supported by the European Research Council/European Community under the FP7 through Starting Grant agreement number 239953. N.C.S. was supported by FCT through the Investigador FCT contract reference IF/00169/2012 and POPH/FSE (EC) by FEDER ...
Mortier, Annelies +18 more
core +1 more source
The effects of stellar winds on the magnetospheres and potential habitability of exoplanets [PDF]
, 2014 V.S. acknowledges the support of an STFC studentship. A.A.V. acknowledges support from a Royal Astronomical Society Fellowship and an Ambizione Fellowship from the Swiss National Science Foundation. S.V.J.
S. C. Marsden +20 more
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