Chemical evolution and galaxy formation
Following a review of the basic ingredients necessary for constructing models of galactic chemical evolution, with a special emphasis on the issue of stellar evolution and nucleosynthesis (which is treated in detail in Chapter 2), I continue with the basic equations that one needs to solve in order to follow the chemical evolution of a system of gas ...
openaire +1 more source
A detailed analysis of the Czernik 38 cluster and its associated tidal tail, utilizing Gaia DR3 and 2MASS. [PDF]
Ahmed NM.
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Genomic Resources for Imperiled Caribbean Reef-Forming Corals (Hexacorallia: Scleractinia): Complete Mitochondrial Genomes of <i>Dichocoenia stokesii</i>, <i>Diploria labyrinthiformis</i>, <i>Oculina patagonica</i>, and <i>Stephanocoenia intersepta</i>. [PDF]
Zabransky K +3 more
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Multiple human enhancer RNAs contain long translated open reading frames. [PDF]
Vlasov PA +5 more
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Beyond the Second Law: Darwinian Evolution as a Tendency for Entropy Production to Increase. [PDF]
Lineweaver CH.
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Discovery of Coerumycin, a Cinnamycin-like Lantibiotic from Actinomadura coerulea TMS085. [PDF]
Iliasov D, Mascher T.
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The emergence of globular clusters and globular-cluster-like dwarfs. [PDF]
Taylor ED +9 more
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Oxygen Binding Kinetics and Coordination States of Hemoglobins from Early Land Plants. [PDF]
Dvorak S, Monroe JD, Hanson K, Sturms R.
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The photometry and kinematics studies of NGC 2509 derived from Gaia DR3. [PDF]
Ahmed NM, Tadross AL.
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Electromagnetic follow-up of gravitational waves: review and lessons learned. [PDF]
Nicholl M, Andreoni I.
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