Results 71 to 80 of about 195,665 (278)

The building up of the disk galaxy M33 and the evolution of the metallicity gradient

, 2007
The evolution of radial gradients of metallicity in disk galaxies and its relation with the disk formation are not well understood. Theoretical models of galactic chemical evolution make contrasting predictions about the time evolution of metallicity ...
Aller, Arnett, Aubert, Beaulieu, Block, Block, Brooks, Bullock, Chabrier, Chang, Chiappini, Chiappini, Chiappini, Chieffi, Ciardullo, Ciardullo, Corbelli, Corbelli, Crockett, D. Galli, Davidge, de Boer, Devereux, Diaz, E. Corbelli, Elmegreen, Engargiola, Ferrini, Ferrini, Ferrini, Ferrini, Freedman, Freeman, Friel, Gallagher, Galletti, Garnett, Gavilán, Goetz, Henry, Henry, Henry, Herrero, Herwig, Heyer, Hippelein, Hirschi, Holmberg, Hoopes, Hou, Israel, Kennicutt, Kennicutt, Kennicutt, Keres, Kim, Koeppen, Kroupa, Kroupa, Kwitter, L. Magrini, Maciel, Maciel, Maciel, Maciel, Magrini, Magrini, Magrini, Marigo, McCarthy, McConnachie, Mollà, Mollà, Mollà, Monteverde, Monteverde, Naab, Newton, Portinari, Portinari, Regan, Richer, Romano, Rowe, Salpeter, Sandage, Scalo, Scalo, Smith, Stanghellini, Stephens, Talbot, Thielemann, Tiede, Tinsley, Tosi, Urbaneja, Venn, Vílchez, Wakker, Westmeier, Willner, Woosley, Wyse, Young   +104 more
core   +1 more source

Simulating an isolated dwarf galaxy with multichannel feedback and chemical yields from individual stars [PDF]

Monthly notices of the Royal Astronomical Society, 2018
In order to better understand the relationship between feedback and galactic chemical evolution, we have developed a new model for stellar feedback at grid resolutions of only a few parsecs in global disk simulations, using the adaptive mesh refinement ...
A. Emerick, G. Bryan, Mordecai-Mark Mac Low   +2 more
semanticscholar   +1 more source

EMPRESS. XIII. Chemical Enrichment of Young Galaxies Near and Far at z ∼ 0 and 4–10: Fe/O, Ar/O, S/O, and N/O Measurements with a Comparison of Chemical Evolution Models

The Astrophysical Journal
We present gas-phase elemental abundance ratios of thirteen local extremely metal-poor galaxies (EMPGs), including our new Keck/LRIS spectroscopy determinations together with 33 James Webb Space Telescope z ∼ 4–10 star-forming galaxies in the literature,
Kuria Watanabe, Masami Ouchi, Kimihiko Nakajima, Yuki Isobe, Nozomu Tominaga, Akihiro Suzuki, Miho N. Ishigaki, Ken’ichi Nomoto, Koh Takahashi, Yuichi Harikane, Shun Hatano, Haruka Kusakabe, Takashi J. Moriya, Moka Nishigaki, Yoshiaki Ono, Masato Onodera, Yuma Sugahara   +16 more
doaj   +1 more source

Chemical Evolution of Galaxies and Intracluster Medium [PDF]

, 2002
In this series of lectures I discuss the basic principles and the modelling of the chemical evolution of galaxies. In particular, I present models for the chemical evolution of the Milky Way galaxy and compare them with the available observational data.
F. Matteuccí
openalex   +4 more sources

Inflow, Outflow, Yields, and Stellar Population Mixing in Chemical Evolution Models [PDF]

, 2016
Chemical evolution models are powerful tools for interpreting stellar abundance surveys and understanding galaxy evolution. However, their predictions depend heavily on the treatment of inflow, outflow, star formation efficiency (SFE), the stellar ...
B. Andrews, D. Weinberg, R. Schönrich, Jennifer A. Johnson   +3 more
semanticscholar   +1 more source

Dust-regulated galaxy formation and evolution:A new chemodynamical model with live dust particles

, 2015
Interstellar dust plays decisive roles in the conversion of neutral to molecular hydrogen (H_2), the thermodynamical evolution of interstellar medium (ISM), and the modification of spectral energy distributions (SEDs) of galaxies.
Bekki, Kenji
core   +1 more source

Galaxy simulation with the evolution of grain size distribution [PDF]

Monthly notices of the Royal Astronomical Society, 2019
We compute the evolution of interstellar dust in a hydrodynamic simulation of an isolated disc galaxy. We newly implement the evolution of full grain size distribution by sampling 32 grid points on the axis of the grain radius. We solve it consistently
S. Aoyama, H. Hirashita, K. Nagamine
semanticscholar   +1 more source

Chemical Evolution of Galaxies

, 1987
We review some of the present ideas on chemical evolution of irregular galaxies and disks of spiral galaxies. Based on the O abundances in stars and H II regions we present a discussion of the yield; we also discuss the effects of large scale mass flows and of cold dark matter to explain variations in the observed yield. The C, N, O observed abundances
Manuel Peimbert, Silvia Torres-Peimbert
openaire   +2 more sources

Modeling the Ages and Chemical Abundances of Elliptical Galaxies

The Astrophysical Journal
Spectroscopic studies of elliptical galaxies show that their stellar population ages, mean metallicity, and α enhancement traced by [Mg/Fe] all increase with galaxy stellar mass or velocity dispersion.
Nicole Marcelina Gountanis, David H. Weinberg, Aliza G. Beverage, Nathan R. Sandford, Charlie Conroy, Mariska Kriek   +5 more
doaj   +1 more source

A chemical evolution model for galaxy clusters [PDF]

, 2001
We develop a toy-model for the chemical evolution of the intracluster medium, polluted by the galactic winds from elliptical galaxies. The model follows the "galaxy formation history" of cluster galaxies, constrained by the observed luminosity function ...
Chiosi, C., Moretti, A., Portinari, L.
core   +1 more source