The solar system is apparently stratified with regard to the contents of volatile constituents, as judged from the rocky, volatile-poor inner solar system planets and meteorites and the huge volatile-rich outer planets. However, beyond this gross structure there is no evidence for a systematic increase of the volatiles' abundances with distance from the Sun. CiteSeerX Elemental Abundances in the X-Ray Gas of Early CiteSeerX - Document Details (Isaac Councill, Lee Giles, Pradeep Teregowda):The source of hot gas in elliptical galaxies is thought to be due to stellar mass loss, with contributions from supernova events and possibly from infall from a surrounding environment. This picture predicts supersolar values for the metallicity of the gas toward the inner part of the galaxy, which can be tested by
Anders E, Ebihara M (1982) Solar system abundances of the elements. Geochim Cosmochim Acta 46:23632380. Google Scholar . Bodinier JL, Guiraud M, Fabriès J, Dostal J, Dupuy C (1987) Petrogenesis of layered pyroxenites from the Lherz, Freychinède and Prades ultramafic bodies (Ariège, French Pyrénées). Iron and Alpha Element Abundances in the Outer Disk, the inner halo (this work) and outer halo . The metal-rich (> -1.5 dex), inner halo (< 26 kpc) is inconsistent with having formed from progenitors similar to present day M31 satellite galaxies (). The outer disk is highly -enhanced (0.60 dex), supporting a Nucleosynthesis and the Origin of the ElementsStellar Nucleosynthesis - Elemental Abundances in the Solar System -4-2 0 2 4 6 8 10 12 1 5 9 13 17 21 25 29 33 37 41 45 49 53 57 61 65 69 73 77 81 Atomic Number e H He Li Be Fe B Sc Big Bang Stellar Nucleo. Supernova Mass-5 (Be) and mass-8 (O) bottleneck
Sep 20, 2017 · The four most abundant elements (O, Mg, Si, and Fe) make up 94.19% of the total primitive mantle mass. SDSS-III:Massive Spectroscopic Surveys of the Distant inner Galaxy from our view, measuring radial velocities, spectral types, and detailed elemental abundances of 100,000 red giant stars to a magnitude limit H 13:5, across the full range of the Galactic bulge, bar, and disk. Together, SEGUE-2 and APOGEE will provide a picture of Study Chapter 20:The Milky Way - A Normal Spiral Galaxy => There is a smooth decline in abundances of massive elements from the inner to the outer parts of the disk. Within the galaxy disk, relatively old stars near the center of a galaxy often have greater massive-element abundances than those of young stars in the outer parts of the disk.
We also assembled from the literature all available optical/near-IR line fluxes of the inner ring. The observed line light curves were then compared with a photoionisation model for the inner ring. This indicates an iron abundance of (0.20±0.08) × solar which is lower than that generally seen in the Large Magellanic Cloud (LMC). 1 The elemental abundances (with uncertainties) of the most Jan 01, 2018 · From a heterogeneous set of literature values, we present the most complete lists of the elemental abundances with uncertainties of the primitive mantle (PM), the core and the bulk Earth ( Table 1, Table 1, Fig. 2, Fig. 3, Fig. 4, Fig. 6, Fig. 7 ). The four most abundant elements (O, Mg, Si, and Fe) make up 94.19 ± 0.69% of the total PM mass. The elemental abundances (with uncertainties) of the most Unlike previous efforts, the uncertainty on the core mass fraction is propagated to the uncertainties on the bulk Earth elemental abundances. Our concordance estimates for the abundances of Mg, Sn, Br, B, Cd and Be are significantly lower than previous estimates of the bulk Earth. Our concordance estimates for the abundances of Na, K, Cl, Zn, Sr, F, Ga, Rb, Nb, Gd, Ta, He, Ar, and Kr are significantly higher.
Sep 01, 2020 · PDF We present measurements of [Fe/H] and [/Fe] for 128 individual red giant branch stars (RGB) in the stellar halo of M31, including its Giant Find, read and cite all the research you