Relative frequencies of Type Ia and Type II supernovae in the chemical evolution of the Galaxy, LMC and SMC
T. Tsujimoto,K. Nomoto,Yuzuru Yoshii,Masa-aki Hashimoto,S. Yanagida,Friedrich-Karl Thielemann +5 more
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This article is published in Monthly Notices of the Royal Astronomical Society.The article was published on 1995-12-01 and is currently open access. It has received 408 citations till now. The article focuses on the topics: Galaxy merger & Interacting galaxy.read more
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The Star formation history of field galaxies
TL;DR: In this paper, the authors developed a method for interpreting faint galaxy data which focuses on the integrated light radiated from the galaxy population as a whole by tracing the evolution with cosmic time of the galaxy luminosity density, as determined from several deep spectroscopic samples.
Journal ArticleDOI
Nucleosynthesis in Chandrasekhar Mass Models for Type Ia Supernovae and Constraints on Progenitor Systems and Burning-Front Propagation
Koichi Iwamoto,F. Brachwitz,Ken'ichi Nomoto,N. Kishimoto,Hideyuki Umeda,W. Raphael Hix,Friedrich-Karl Thielemann,Friedrich-Karl Thielemann +7 more
TL;DR: In this paper, the authors calculate explosive nucleosynthesis in relatively slow deflagrations with a variety of deflagration speeds and ignition densities to put new constraints on the above key quantities.
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Star-Formation Histories, Abundances, and Kinematics of Dwarf Galaxies in the Local Group
TL;DR: A review of the results of quantitative studies in nearby dwarf galaxies can be found in this paper, where the combination of spectroscopy and imaging and what they have taught us about dwarf galaxy formation and evolution is the aim of this work.
Journal ArticleDOI
Stellar chemical signatures and hierarchical galaxy formation
Kim A. Venn,Kim A. Venn,Kim A. Venn,Mike Irwin,Matthew Shetrone,Christopher A. Tout,Vanessa Hill,Eline Tolstoy +7 more
TL;DR: In this paper, the authors compared the chemistries of stars in the Milky Way dwarf spheroidal (dSph) satellite galaxies with stars from the Galaxy, and found that the [α/Fe] ratios of most stars in dSph galaxies are generally lower than similar metallicity Galactic stars in this extended sample.
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alpha-, r-, and s-process element trends in the Galactic thin and thick disks
TL;DR: Bensbyet et al. as discussed by the authors presented abundance trends in the Galactic thin and thick disks for 14 elements (O, Na, Mg, Al, Si, Ca, Ti, Cr, Fe, Ni, Zn, Y, Ba, and Eu).
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