Results 61 to 70 of about 50,982 (241)
Evolution of Li, Be and B in the Galaxy [PDF]
In this paper we study the production of Li, Be and B nuclei by Galactic cosmic ray spallation processes. We include three kinds of processes: (i) spallation by light cosmic rays impinging on interstellar CNO nuclei (direct processes); (ii) spallation by
Bonifacio P. +20 more
core +2 more sources
Helium Abundance at the Galactic Center
We suggest that the low abundance of ionized helium in H II regions at the galactic center can be explained by selective absorption of helium-ionizing photons by dust within the ionized gas. This model requires an extrapolation to 500 A of the rapid increase of the extinction measured between 1500 A and 1000 A with the Copernicus satellite, and it ...
E. L. Wright, M. Jura
openaire +2 more sources
Abundances of Chemical Elements in Open Star Clusters as Indicators of their Nature
Applying a compilled catalog, we find that the relative abundances of α-elements in open clusters and in field stars of the thin disk of the Galaxy show different dependencies on metallicity, age and parameters of their Galactic orbits.
Marsakov V. A. +3 more
doaj +1 more source
Constraining planet structure and composition from stellar chemistry: trends in different stellar populations [PDF]
The chemical composition of stars that have orbiting planets provides important clues about the frequency, architecture, and composition of exoplanet systems.
Adibekyan, V. +10 more
core +2 more sources
Abundances and Evolution of Lithium in the Galactic Halo and Disk [PDF]
We have measured the Li abundance of 18 stars with -2 -0.5. We speculate that cool-bottom processing (production) of Li in low-mass stars may provide an important late-appearing source of Li, without attendant Fe production, that might explain the Li production in the young disk.
Timothy C. Beers +7 more
openaire +4 more sources
We conducted an analysis of the abundances of He, C, and N in 210 He-rich hot subdwarfs observed within both the Gaia Data Release 3 (DR3) and LAMOST DR7 data sets.
Yangping Luo +3 more
doaj +1 more source
MOLYBDENUM AND RUTHENIUM ABUNDANCES IN COOL STARS OF THE GALACTIC DISC
We revise the molybdenum and ruthenium abundances in FGK stars with metallicities ranging from −1.0 < [Fe/H] < +0.3. The observed stars belong to the substructures of the Galaxy. The observations were conducted using the 1.93 m telescope at
T. I. Gorbaneva, T. V. Mishenina
doaj +1 more source
Determination of Abundances of Chemical Elements in Open Star Clusters of the Galaxy
Spectroscopic determinations of the relative abundances of chemical elements produced in different nuclear-synthesis processes, [el/Fe], are collected for 90 open star clusters of the Galaxy using data from 109 papers published between 1991 and 2015 ...
Gozha M. L. +2 more
doaj +1 more source
Mn abundances in the stars of the Galactic disc with metallicities -1.0 < [Fe/H] < 0.3 [PDF]
In this work we present and discuss the observations of the Mn abundances for 247 FGK dwarfs, located in the Galactic disc with metallicity -1 < [Fe/H]< +0.3.
Gorbaneva, Tatyana Ivanovna +4 more
core +2 more sources
On the Abundance Gradient of the Galactic Disk
6 pages, 2 ...
Martins, Lucimara P. +1 more
openaire +2 more sources

