Results 1 to 10 of about 1,649,449 (138)

Modelling the chemical evolution [PDF]

Proceedings of the International Astronomical Union, 2010
Advanced observational facilities allow to trace back the chemical evolution of the Universe, on the one hand, from local objects of different ages and, secondly, by direct observations of redshifted objects.
Argast, Cescutti, Chiappini, Colavitti, Gerhard Hensler, Harfst, Hensler, Hensler, Hensler, Hensler, Hirschi, Ikuta, Koch, Koeppen, Koeppen, Kroeger, Maciel, Maeder, Matteucci, Meynet, Meynet, Meynet, Momany, Nordstroem, Pagel, Pagel, Portinari, Portinari, Prantzos, Prantzos, Recchi, Recchi, Recchi, Recchi, Revaz, Samland, Schaller, Simone Recchi, Spitoni, Theis, Tinsley   +40 more
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Chemical Evolution in VeLLOs [PDF]

Journal of The Korean Astronomical Society, 2007
A new type of object called "Very Low Luminosity Objects (VeLLOs)" has been discovered by the Spitzer Space Telescope. VeLLOs might be substellar objects forming by accretion.
Lee, Jeong-Eun
core   +4 more sources

The Chemical Evolution of Phosphorus [PDF]

The Astrophysical Journal, 2014
Phosphorus is one of the few remaining light elements for which little is known about its nucleosynthetic origin and chemical evolution, given the lack of optical absorption lines in the spectra of long-lived FGK-type stars.
Cescutti, Gabriele, Frebel, Anna, Jacobson, Heather R., Matteucci, Francesca, Roederer, Ian U., Thanathibodee, Thanawuth   +5 more
core   +4 more sources

Cosmic Chemical Evolution [PDF]

, 1999
Numerical simulations of standard cosmological scenarios have now reached the degree of sophistication required to provide tentative answers to the fundamental question: Where and when were the heavy elements formed? Averaging globally, these simulations
Dave R., Jeremiah P. Ostriker, Renyue Cen, Tamura T., Tripp T. M.   +4 more
core   +2 more sources

Evolution Of Galaxies .2. Chemical Evolution Coefficients [PDF]

, 1973
NSF GP-18355, GP ...
Arnett, W. David, Talbot, Raymond. J.
core   +1 more source

The chemical evolution of IC 10 [PDF]

Astronomy and Astrophysics, 2010
Dwarf irregular galaxies are relatively simple unevolved objects where it is easy to test models of galactic chemical evolution. We attempt to determine the star formation and gas accretion history of IC10, a local dwarf irregular for which abundance, gas, and mass determinations are available. We apply detailed chemical evolution models to predict the
Yin J., Magrini L., MATTEUCCI, MARIA FRANCESCA, Lanfranchi G. A., Gonçalves D. R., Costa R. D. D.   +5 more
openaire   +3 more sources

Chemical Evolution of Galaxies [PDF]

, 2000
Chemical evolution of galaxies brings together ideas on stellar evolution and nucleosynthesis with theories of galaxy formation, star formation and galaxy evolution, with all their associated uncertainties.
Arimoto N., Arnaud M., B. E. J. Pagel, Beers T. C., Edvardsson B., Fuhrmann K., Gasson R. E. M., Gratton R., Gustafsson B., Hoyle F., Larson R. B., Madau P., Maeder A., Marigo P., Matteucci F., Nissen P. E., Pagel B. E. J., Pagel B. E. J., Renzini A., Scalo J., Thielemann F.-K., White S. D. M.   +21 more
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Chemical evolution

, 2008
In this series of lectures we first describe the basic ingredients of galactic chemical evolution and discuss both analytical and numerical models. Then we compare model results for the Milky Way, Dwarf Irregulars, Quasars and the Intra-Cluster- Medium with abundances derived from emission lines.
Horst Rauchfuss, Terence N. Mitchell
openaire   +3 more sources

Chemical evolution of Seyfert galaxies [PDF]

, 2007
We computed the chemical evolution of Seyfert galaxies, residing in spiral bulges, based on an updated model for the Milky Way bulge with updated calculations of the Galactic potential and of the feedback from the central supermassive black hole (BH) in ...
Ballero, Francesca Matteucci, Luca Ciotti, Matteucci, Silvia K. Ballero, Wang   +5 more
core   +1 more source

Stellar Chemical Evolution [PDF]

Symposium - International Astronomical Union, 1997
One of the major achievements of astrophysics has been the demonstration that most of the chemical elements have been synthesized in stars: nucleosynthesis calculations of homogeneous and inhomogeneous big bang cosmologies show that, in comparison with the most metal-poor stars currently known, essentially no elements heavier than B existed at the era ...
openaire   +1 more source