Results 231 to 240 of about 195,665 (278)
Comparison of a new type of Dark Matter with the Milky Way and M31 grand rotation curves. [PDF]
Law BM.
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A natural mechanism of eukaryotic horizontal gene transfer
Urquhart AS+3 more
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Infrared Spectroscopy of Pentagon-Containing PAHs: Indenyl and Fluorenyl Anions and Indenyl Cation. [PDF]
Wenzel G+6 more
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AptERA 2 targets ERA from Staphylococcus aureus and limits GTP hydrolysis
Peñaranda K+6 more
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Chemical Evolution of the Galaxy
Annual Review of Astronomy and Astrophysics, 1991Standard models for the chemical evolution of the Galaxy are reviewed with particular emphasis on the history of the abundance gradients in the disk.
N. Rana
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Elliptical Galaxy Chemical Evolution [PDF]
Conclusions about elliptical and other early-type galaxies come from studies of integrated starlight and studies of giant stars in the nearest galaxies. The abundance distribution for all galaxy types at all radii appears to exhibit a “G dwarf problem” in that the distribution is more strongly peaked than the one-zone closed-box constantyield ...
G. Worthey
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Chemical Evolution of Galaxies
Annual Review of Astronomy and Astrophysics, 1976The various nucleosynthetic processes needed to account for the formation of the different nuclear species have been described in the previous chapters as well as the location of these nucleosynthetic events. At the beginning of this monograph, the evolution of the matter which constitutes the celestial bodies such as planets, stars and galaxies was ...
Audouze, J., Tinsley, B.M.
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Chemical evolution of the galaxy
AIP Conference Proceedings, 1995The article presents data on and discussion of various issues related to element abundance trends in our Galaxy as a function of metallicity [Fe/H]: halo star abundances, evolution of the Galactic supernova rates, the age‐metallicity relationship for disk stars, and halo and disk star formation history and nycleosynthesis timescales. (AIP)
James W. Truran, Francis Timmes
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The Chemical Evolution of Galaxies
Progress in Particle and Nuclear Physics, 1986After a brief introduction into the evolution of spiral galaxies, the observational evidence for temporal and spatial abundance variations across the galactic disk is discussed. The theoretical framework of chemical evolution models is summarised, followed by a critical discussion of available constraints. Solutions applying to the special cases of the
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