Results 91 to 100 of about 426,951 (145)
From the s-Process to the i-Process: A New Perspective on the Chemical Enrichment of Extrinsic Stars
Separating stars enriched in the s- and r-processes of nucleosynthesis is usually achieved by analyzing the element ratios of s-process elements (like Ba or La) to r-process elements (like Eu).
Sophie Van Eck +11 more
doaj +1 more source
Abstract Nearshore seagrass, kelp, and other macroalgae beds (submerged aquatic vegetation [SAV]) are productive and important ecosystems. Mitigating anthropogenic impacts on these habitats requires tools to quantify their ecological value and the debits and credits of impact and mitigation.
Rachel E. Pausch +10 more
wiley +1 more source
Eridanus III and DELVE 1: Carbon-rich Primordial Star Clusters or the Smallest Dwarf Galaxies?
We present spectroscopy of the ultra-faint Milky Way satellites Eridanus III (Eri III) and DELVE 1. We identify eight member stars in each satellite and place nonconstraining upper limits on their velocity and metallicity dispersions.
Joshua D. Simon +10 more
doaj +1 more source
ABSTRACT The North American boreal forest is a massive ecosystem, and its keystone herbivore is the snowshoe hare (Lepus americanus). Hares are exposed to considerable environmental extremes in diet and weather, food availability, and predation risk.
Mason R. Stothart +7 more
wiley +1 more source
The development of hydrogen gas (H2) therapy is highly challenging by reason of low efficiency and suboptimal utilization due to its high diffusibility, nonpolarity, and low solubility of H2 in physiological conditions, which prevent long‐term release and reduce therapeutic efficiency.
Yingyi Zhang +15 more
wiley +1 more source
Carbon-Enhanced Metal-Poor (CEMP) stars [PDF]
AbstractA significant fraction of metal-poor stars have large over-abundances of carbon, and are called Carbon-Enhanced Metal-Poor (CEMP) stars. Most of CEMP stars also show excesses of heavy neutron-capture elements like Ba, indicating that their origin is the nucleosynthesis in AGB stars.
openaire +1 more source
Modelling the observed properties of carbon-enhanced metal-poor stars using binary population synthesis [PDF]
The stellar population in the Galactic halo is characterised by a large fraction of carbon-enhanced metal-poor (CEMP) stars. Most CEMP stars have enhanced abundances of s-process elements (CEMP-s stars), and some of these are also enriched in r-process ...
Karakas, A. I. +6 more
core +2 more sources
JCVI: A versatile toolkit for comparative genomics analysis
The JCVI library contains a set of computational tools that are often used in tasks covering genome assembly, annotation, and comparative genomics. Engineered with a focus on versatility, the library incorporates modules for algorithms, format parsing, and graphics generation, enabling seamless integration into diverse research workflows.
Haibao Tang +11 more
wiley +1 more source
Three extremely metal-poor stars: discovery of a new CEMP-no star
ABSTRACT We have conducted detailed high-resolution spectroscopic studies on three extremely metal-poor (EMP) stars HE 0401–0138, HE 1153–0518, and HE 1246–1344. For the stars HE 0401–0138 and HE 1246–1344, we have estimated the abundances of C, Na, Mg, Ca, Sc, Ti, Cr, Mn, Co, Ni, Sr, and Ba along with the upper limits for Li, O, La ...
Goswami, Partha Pratim, Goswami, Aruna
openaire +2 more sources
Evaluating Classifications of Extremely Metal-poor Candidates Selected from Gaia XP Spectra
Extremely metal-poor stars are intrinsically rare, but emerging methods exist to accurately classify them from all-sky Gaia XP low-resolution spectra.
Riley Thai +4 more
doaj +1 more source

