Results 41 to 50 of about 694,028 (301)

THE STARS OF THE LOWER PART OF MAIN SEQUENCE

open access: yesOdessa Astronomical Publications, 2007
Atmospheric parameters (Teff , log g, [Fe/H], Vt), Li, and volatile (O, Na, Al, Zn) and refractory (Si, Ti, V, Cr, Co and Ni) element abundances in 133 stars belonging to the low part of MS have been determined. Among them about 30 stars are the variable
T. V. Mishenina   +6 more
doaj   +1 more source

Lithium abundances in extremely metal-poor unevolved stars

open access: yes, 2005
Lithium abundance, metal-poor stars, VLT/UVES ...
Andersen, Johannes   +10 more
core   +1 more source

A Systematic NLTE Study of Very Metal-poor Stars with Metallicity Down to −4.3 dex. II. Lithium Abundance and New Insight of the Lithium Plateau

open access: yesThe Astrophysical Journal
Metal-poor stars are crucially important for understanding the early Galaxy, first stars, and the Universe. In this series of papers, we present a homogeneous non–local thermodynamic equilibrium (NLTE) abundance analysis of 12 elements for 103 very metal-
Hong-Liang Yan   +14 more
doaj   +1 more source

Counterion Dependent Side‐Chain Relaxation Stiffens a Chemically Doped Thienothiophene Copolymer

open access: yesAdvanced Functional Materials, EarlyView.
Oxidation of a thienothiophene copolymer, p(g3TT‐T2), via different doping strategies and dopant molecules resulted in materials with similar oxidation levels and a high electrical conductivity of ≈100 S cm−1. However, mechanical properties varied significantly, with sub‐glass transition temperatures and elastic moduli spanning from –44°C to –3°C and ...
Mariavittoria Craighero   +12 more
wiley   +1 more source

Lithium in the closest satellite of our Milky Way

open access: yes, 2020
Recently, we studied the chemical evolution of lithium in the thin disc of the Milky Way. We found that the best agreement with the observed Li abundances in the thin disc is obtained considering novae as the main source of lithium.
P. Molaro, X. Fu, G. Cescutti
core   +1 more source

Lithium Abundances from the LAMOST Medium-resolution Survey Data Release 9

open access: yesThe Astrophysical Journal Supplement Series
Lithium is a fragile but crucial chemical element in the Universe, and exhibits interesting and complex behaviors. Thanks to the mass of spectroscopic data from the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) medium-resolution ...
Ming-Yi Ding   +11 more
doaj   +1 more source

From Food to Power: Hydrogel Thermoelectrics for Ingestible Electronics

open access: yesAdvanced Functional Materials, EarlyView.
We introduce a fully edible thermoelectric–electrochromic platform that harvests heat from food and converts it into a visible color change. N‐type and p‐type hydrogel thermoelectric generators connected in series power anthocyanin‐based electrochromic displays, demonstrating the feasibility of safe, biodegradable, ingestible systems for on‐food ...
Antonia Georgopoulou   +3 more
wiley   +1 more source

The lithium isotopic ratio in very metal-poor stars [PDF]

open access: yes, 2016
Context. Un-evolved, very metal-poor stars are the most important tracers of the cosmic abundance of lithium in the early universe. Combining the standard Big Bang nucleosynthesis model with Galactic production through cosmic ray spallation, these stars
Asplund, Martin   +4 more
core   +1 more source

Regulated Ion‐Diffusion Hydrogels for Subtle and Multimodal Temperature‐Strain Sensing in Wound Monitoring

open access: yesAdvanced Functional Materials, EarlyView.
A soft, dual‐channel hydrogel patch enables simultaneous detection of wound temperature and strain by integrating ion‐diffusion‐mediated thermoelectric and resistive sensing. The conformal design maintains stable performance during motion, capturing subtle inflammatory and mechanical changes for continuous wound monitoring.
Yu Fang   +7 more
wiley   +1 more source

Lithium abundances in metal-poor stars

open access: yes, 1999
We present the lithium measurements of a continuing programme of light element abundances in metal-poor stars. New equivalent widths of the Li 
P. François   +4 more
core   +1 more source

Home - About - Disclaimer - Privacy