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相关论文: Cosmological evolution of metallicity correlation …

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We study the relation between the metallicities of ionised and atomic gas in star-forming galaxies at z=0-3 using the EAGLE cosmological, hydrodynamical simulations. This is done by constructing a dense grid of sightlines through the…

The gas-phase metallicity of galaxies is regulated by multiple astrophysical processes, which makes it a crucial diagnostic of galaxy formation and evolution. Beyond the fundamental mass-metallicity relation, a debate about the secondary…

星系天体物理 · 物理学 2024-08-09 Chengyu Ma , Kai Wang , Enci Wang , Yingjie Peng , Haochen Jiang , Haoran Yu , Cheng Jia , Zeyu Chen , Haixin Li , Xu Kong

We study the gas metallicity of quasar hosts using cosmological hydrodynamic simulations of the Lambda-cold dark matter model. Galaxy formation in the simulations is coupled with a prescription for black hole activity enabling us to study…

天体物理学 · 物理学 2009-11-10 Tiziana Di Matteo , Rupert A. C. Croft , Volker Springel , Lars Hernquist

We explore the origin of stellar metallicity gradients in simulated and observed dwarf galaxies. We use FIRE-2 cosmological baryonic zoom-in simulations of 26 isolated galaxies as well as existing observational data for 10 Local Group dwarf…

Tracing the cosmic path of galaxies requires an understanding of their chemical enrichment and merging histories. One of the most important constraints is the internal structure of galaxies, notably the internal distribution of elements…

星系天体物理 · 物理学 2025-10-14 Dyna Ibrahim , Chiaki Kobayashi

The metallicity gradients of the stellar populations in disc galaxies and their evolution store relevant information on the disc formation history and on those processes which could mix stars a posteriori, such as migration, bars and/or…

In order to recognize environmental effects on the evolution of dwarf galaxies in clusters of galaxies, it is first necessary to quantify the properties of objects which have evolved in relative isolation. With oxygen abundance as the gauge…

天体物理学 · 物理学 2009-11-07 Henry Lee , Marshall L. McCall , Robin L. Kingsburgh , Robert Ross , Chris C. Stevenson

We present preliminary results of an ESO-VLT large programme (AMAZE) aimed at determining the evolution of the mass-metallicity relation at z~3 by means of deep near-IR spectroscopy. Gas metallicities and stellar masses are measured for an…

We present and discuss measurements of the gas-phase metallicity gradient in gravitationally lensed galaxies at z=2.0-2.4 based on adaptive optics-assisted imaging spectroscopy with the Keck II telescope. Through deep exposures we have…

宇宙学与河外天体物理 · 物理学 2015-06-05 Tucker Jones , Richard S. Ellis , Johan Richard , Eric Jullo

We present an analytic formalism that describes the evolution of the stellar, gas, and metal content of galaxies. It is based on the idea, inspired by hydrodynamic simulations, that galaxies live in a slowly-evolving equilibrium between…

宇宙学与河外天体物理 · 物理学 2015-05-30 Romeel Davé , Kristian Finlator , Benjamin D. Oppenheimer

Metallicity is one of the crucial factors that determine stellar evolution. To characterize the properties of stellar populations one needs to know the fraction of stars forming at different metallicities. Knowing how this fraction evolves…

星系天体物理 · 物理学 2019-07-29 Martyna Chruslinska , Gijs Nelemans

We present the mass-metallicity (MZ) and luminosity-metallicity (LZ) relations at z ~ 0.8 from ~1350 galaxies in the Deep Extragalactic Evolutionary Probe 2 (DEEP2) survey. We determine stellar masses by fitting the spectral energy…

宇宙学与河外天体物理 · 物理学 2015-05-19 H. J. Zahid , L. J. Kewley , F. Bresolin

The metal content of galaxies provides a window into their formation in the full context of the cosmic baryon cycle. In this study, we examine the relationship between stellar mass and stellar metallicity (${\rm MZ}_*{\rm R}$) in the…

During the last three decades, many papers have reported the existence of a luminosity-metallicity or mass-metallicity (M-Z) relation for all kinds of galaxies: The more massive galaxies are also the ones with more metal-rich interstellar…

宇宙学与河外天体物理 · 物理学 2019-08-15 N. Vale Asari , G. Stasinska , R. Cid Fernandes , J. M. Gomes , M. Schlickmann , A. Mateus , W. Schoenell

We present the time evolution of the stellar metallicity for SDSS galaxies, a sample that spans five orders of magnitude in stellar mass (10^7 - 10^{12} Msun). Assuming the BC03 stellar population models, we find that more massive galaxies…

天体物理学 · 物理学 2009-11-13 Benjamin Panter , Raul Jimenez , Alan F. Heavens , Stephane Charlot

In their evolution, star-forming galaxies are known to follow scaling relations between some fundamental physical quantities, such as the mass-metallicity and the main sequence relations. We aim at studying the evolution of galaxies that,…

星系天体物理 · 物理学 2020-10-14 E. Spitoni , F. Calura , M. Mignoli , R. Gilli , V. Silva Aguirre , A. Gallazzi

We analyse the metallicity histories of ~4,500 galaxies from the GAMA survey at z<0.06 modelled by the SED-fitting code ProSpect using an evolving metallicity implementation. These metallicity histories, in combination with the associated…

We present results from deep Spitzer/Infrared Array Camera (IRAC) observations of 28 metal-poor, strongly star-forming galaxies selected from the DEEP2 Galaxy Survey. By modelling infrared and optical photometry, we derive stellar masses…

星系天体物理 · 物理学 2020-01-08 Andrew Weldon , Chun Ly , Michael Cooper

Metallicity and gas content are intimately related in the baryonic exchange cycle of galaxies, and galaxy evolution scenarios can be constrained by quantifying this relation. To this end, we have compiled a sample of ~400 galaxies in the…

星系天体物理 · 物理学 2020-06-10 Michele Ginolfi , Leslie K. Hunt , Crescenzo Tortora , Raffaella Schneider , Giovanni Cresci

Using the FIRE-2 cosmological zoom-in simulations, we investigate the temporal evolution of gas-phase metallicity radial gradients of Milky Way-mass progenitors in the redshift range of $0.4<z<3$. We pay special attention to the occurrence…