Results 51 to 60 of about 426,951 (145)
Carbon measurements in two ultra-faint dwarf galaxies: Grus II and Tucana IV
The ultra-faint dwarf galaxies (UFDs) are some of the oldest and most metal-poor environments in the Local Group. In particular, they are predicted to host the first stars (only H and He) that lit up in our Universe.
Verdiani Valentina +9 more
doaj +1 more source
Abstract figure legend During GLP‐1RA treatment reduced appetite and energy intake, delayed gastric emptying, decreased visceral fat mass and improved glycaemic control contribute to weight loss. After treatment cessation these benefits are partially or completely reversed, resulting in weight regain, accompanied by increased appetite and energy intake,
Camille E. M. Piguet +2 more
wiley +1 more source
The Spatiotemporal Genetic Architecture of Seed Vigor in Upland Cotton
Leveraging the semi‐automated SeedRanger platform, we profiled the germination kinetics of 356 cotton accessions at a 30‐min interval. This high‐throughput phenomic approach delineated a temporal genetic network comprising 541 stage‐specific loci. Crucially, functional validation identified FLA2 as a pivotal, auxin‐modulated regulator that orchestrates
Luyao Wang +32 more
wiley +1 more source
Origin of CEMP stars: What helium and lithium can tell us about CEMP stars?
We show that the peculiar surface abundance patterns of Carbon Enhanced Metal Poor (CEMP) stars has been inherited from material having been processed by H- and He-burning phases in a previous generation of stars (hereafter called the ``Source Stars'').
Meynet, Georges +6 more
openaire +2 more sources
Discovery of the First Five Carbon-enhanced Metal-poor Stars in the LMC
A substantial fraction of metal-poor stars in the local Milky Way halo exhibit large overabundances of carbon. These stars, dubbed carbon-enhanced metal-poor (CEMP) stars, provide crucial constraints on the nature of the early Universe, including the ...
Madeline Lucey +9 more
doaj +1 more source
Biosynthesis and accumulation of tanshinones in the periderm of Salvia miltiorrhiza during secondary root growth. Summary Perennial herbs develop long‐lived roots that undergo repeated cycles of secondary growth, during which the periderm functions as a protective barrier and a major site of specialized metabolite accumulation.
Licheng Liu +19 more
wiley +1 more source
In this work, we study the phase-space and chemical properties of the Sagittarius (Sgr) stream, the tidal tails produced by the ongoing destruction of the Sgr dwarf spheroidal (dSph) galaxy, focusing on its very metal-poor (VMP; [Fe/H] < −2) content.
Guilherme Limberg +8 more
doaj +1 more source
Origins of carbon-enhanced metal-poor stars [PDF]
We investigate the nature of carbon-enhanced metal-poor (CEMP) stars in Milky Way (MW) analogues selected from the eagle cosmological hydrodynamical simulation.
Cooke, Ryan J. +7 more
core +1 more source
A New Subclass of Carbon-enhanced Metal-poor Stars at Extremely Low Metallicity
We report the discovery of a new subclass of carbon-enhanced metal-poor (CEMP) stars, characterized by high absolute carbon abundances ( A (C) > 7.39) and extremely low metallicity ([Fe/H] ≤ –3.1) but notably lacking enhancements in neutron-capture ...
Young Sun Lee +6 more
doaj +1 more source
Abstract Substantial individual variation in diet and foraging strategies can exist within populations. These differences can enhance individual foraging efficiency, reduce intraspecific competition, and provide fitness advantages that increase the resilience of a population.
Noémie Friscourt +10 more
wiley +1 more source

