Results 1 to 10 of about 58,640 (235)
Chemical Evolution of Galaxies [PDF]
Publications of the Astronomical Society of the Pacific, 2001 SUMMARYThis paper discusses the initial mass function, the oxygen yield and the helium abundance in irregular and blue compact galaxies.
B. E. J. Pagel
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Disk Galaxy Models Driven by Stochastic Self-Propagating Star Formation
Open Astronomy, 2010 We present a model of chemical and spectrophotometric evolution of disk galaxies based on a stochastic self-propagating star formation scenario. The model incorporates galaxy formation through the process of accretion, chemical and photometric evolution ...
Mineikis T., Vansevičius V.
doaj +3 more sources
Modeling the chemical evolution of the Galaxy halo [PDF]
Astronomy & Astrophysics, 2013 We study the chemical evolution and formation of the Galactic halo through the analysis of its stellar metallicity distribution function and some key elemental abundance patterns. Starting from the two-infall model for the Galaxy, which predicts too few low-metallicity stars, we add a gas outflow during the halo phase with a rate proportional to the ...
Francesca Matteucci +3 more
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Chemical Evolution of the Galaxy
, 1994 ten pages in CUPstyle LaTex: extract at the end the corresponding confguid ...
M. Tosi
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PN-Carbon Yields and the Chemical Evolution of the Galaxy [PDF]
, 2001 Two sets of observational carbon stellar yields for low-and-intermediate mass stars are computed from planetary nebulae abundances derived from C II $\lambda4267$ and C III $\lambda\lambda1906+1909$ lines, respectively.
Leticia Carigi
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Evolution of chemical abundances in Seyfert galaxies [PDF]
Astronomy & Astrophysics, 2007 17 pages, 15 figures, 3 tables, accepted for publication in A& ...
S. K. Ballero +4 more
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The Chemical Evolution of Galaxy Disks
, 2000 We discuss the main ingredients necessary to build models of chemical evolution of spiral galaxies and in particular the Milky Way galaxy. These ingredients include: the star formation rate, the initial mass function, the stellar yields and the gas flows.
F. Matteuccí
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Chemical Evolution of Clusters of Galaxies
, 2001 The high metallicity of the intra-cluster medium (ICM) is generally interpreted on the base of the galactic wind scenario for elliptical galaxies. In this framework, we develop a toy-model to follow the chemical evolution of the ICM, formulated in analogy to chemical models for individual galaxies.
L. Portinari, A. Moretti, C. Chiosi
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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
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Chemical and mass evolution of galaxies
, 2004 6 pages, needs saltwshop.sty; to appear in: ``First Robert Stobie SALT Workshop", Science with SALT Workshop Proceedings, Vol. 2, ed. D. A. H.
B. Ziegler
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