Results 61 to 70 of about 65,258,316 (368)
Detailed homogeneous abundance studies of 14 Galactic s-process enriched post-AGB stars: In search of lead (Pb) [PDF]
, 2015 Context. This paper is part of a larger project in which we systematically study the chemical abundances of Galactic and extragalactic post-asymptotic giant branch (post-AGB) stars.
K. D. Smedt +6 more
semanticscholar +1 more source
Multidimensional process mining using process cubes [PDF]
, 2015 Process mining techniques enable the analysis of processes using event data. For structured processes without too many variations, it is possible to show a relative simple model and project performance and conformance information on it. However, if there
Bolt, A. +6 more
core +1 more source
Colloids and Interfaces, 2023 A lot of applications for (semi-)crystalline triacylglycerol (TAG)-in-water dispersions exist in the life science and pharmaceutical industries.
Jasmin Reiner +3 more
doaj +1 more source
To Ba or not to Ba: Enrichment in s-process elements in binary systems with WD companions of various masses [PDF]
, 2015 Context. The enrichment in s-process elements of barium stars is known to be due to pollution by mass transfer from a companion formerly on the thermally-pulsing asymptotic giant branch (AGB), now a carbon-oxygen white-dwarf (WD). Aims.
T. Merle +5 more
semanticscholar +1 more source
Foods, 2020 Moringa oleifera is originally a tropical crop with a fast development, little known in developed countries but cultivated since ancient times. It can adapt to regions affected by climate change, such as the Mediterranean basin, since it is a crop with a
Carla Trigo +4 more
doaj +1 more source
Broad levels in 17 O and their relevance for the astrophysical s process [PDF]
, 2015 Levels in $^{17}$O affect the astrophysical s-process in two opposite ways. The neutron production is enhanced by resonances in the $^{13}$C($\alpha$,$n$)$^{16}$O reaction at excitation energies around 7 MeV in $^{17}$O, and the number of available ...
T. Faestermann +3 more
semanticscholar +1 more source
The Ongoing Deep Underground Measurement of 22Ne(α,n)25Mg at the Ion Beam Facility of the INFN-LNGS
GalaxiesThe 22Ne(α,n)25Mg reaction is of major importance in nuclear astrophysics. It is the main neutron source for the weak s-process and as such is responsible for the nucleosynthesis of 60 < A < 90 elements.
Andreas Best +2 more
doaj +1 more source
NSAIDs as a Drug Repurposing Strategy for Biofilm Control
Antibiotics, 2020 Persistent infections, usually associated with biofilm-producing bacteria, are challenging for both medical and scientific communities. The potential interest in drug repurposing for biofilm control is growing due to both disinvestment in antibiotic R&D ...
Cláudia Leão +2 more
doaj +1 more source
Energy consumption and carbon footprint of perovskite solar cells
Energy Reports, 2022 Recently, perovskite solar cells (PSCs) emerged and promise to break the prevailing solar energy paradigm by combining both low-cost and high-efficiency.
Ana L. Carneiro +4 more
doaj +1 more source
Probing astrophysically important states in the Mg 26 nucleus to study neutron sources for the s process [PDF]
, 2015 Background: The ²²Ne(α,n) ²⁵Mg reaction is the dominant neutron source for the slow neutron capture process (s process) in massive stars, and contributes, together with C¹³(α,n)O¹⁶, to the production of neutrons for the s process in asymptotic giant ...
R. Talwar +24 more
semanticscholar +1 more source