Results 31 to 40 of about 2,098,248 (309)
FEED CONSUMPTION IN RELATION TO EGG FORMATION AND ENVIRONMENTAL TEMPERATURE IN DANDARAWI AND HY-LINE STRAINS. [PDF]
Journal of Animal and Poultry Production, 2007 A total of one hundred eighty, 40 weeks old from both Dandarawi and Hy-line strains were used in this experiment. Birds within each strain were subdivided into two groups.
M. Abdelnabi,
doaj +1 more source
A Note on the Formation of Stellar Absorption Lines [PDF]
The Astrophysical Journal, 1936 Microphotometer measures of the total absorptions of lines of O II within the wing of Hγ, and of CaH within the wing of HЄ, show departures from the normal absorptions predicted from the multiplet intensities of these lines. The departures increase with the wing absorption, but the effect is more pronounced for O II than for CaH.
Swings, Polydore, Struve, Otto
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Finite-time singularity formation at a magnetic neutral line in Hall magnetohydrodynamics
, 2015 The formation of a current sheet in a weakly collisional plasma can be modelled as a finite-time singularity solution of magnetohydrodynamic equations.
Litvinenko, Yuri E. +3 more
core +1 more source
LINE FORMATION IN SPECTRA OF X-RAY NOVAE
Odessa Astronomical Publications, 2017 Results of X-ray Novae (XN) optical spectra computation are presented. The continuum and Balmer line are calculated. The model of XN as a self-irradiated accretion disk is used.
V. F. Suleimanov, V. V. Shimansky
doaj +1 more source
LIMpy: A Semianalytic Approach to Simulating Multiline Intensity Maps at Millimeter Wavelengths
The Astrophysical Journal, 2023 Mapping of multiple lines such as the fine-structure emission from [C ii ] (157.7 μ m), [O iii ] (52 and 88.4 μ m), and rotational emission lines from CO are of particular interest for upcoming line intensity mapping (LIM) experiments at millimeter ...
Anirban Roy +4 more
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Formation and Stability of Lines Produced by Inkjet Printing [PDF]
Langmuir, 2010 To produce stable lines with parallel sides through inkjet printing, individual drops are deposited on a surface so that they coalesce; this initial liquid line (or bead) must remain stable until it forms a solid. The stable line width is shown to be bounded by two limits, with the lower bound (minimum line width) determined by the maximum drop spacing
Stringer, Jonathan +1 more
openaire +4 more sources
Tie-Line Analysis Reveals Interactions Driving Heteromolecular Condensate Formation
Physical Review X, 2022 Phase separation of biomolecules gives rise to membraneless organelles that contribute to the spatiotemporal organization of the cell. In most cases, such biomolecular condensates contain multiple components, but the manner in which interactions between ...
Daoyuan Qian +8 more
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FEBS Letters, EarlyView.Enteropathogenic E. coli (EPEC) infects the human intestinal epithelium, resulting in severe illness and diarrhoea. In this study, we compared the infection of cancer‐derived cell lines with human organoid‐derived models of the small intestine. We observed a delayed in attachment, inflammation and cell death on primary cells, indicating that host ...
Mastura Neyazi +5 more
wiley +1 more source
Taming contact line instability for pattern formation
Nature Communications, 2016 Coating flows on surfaces are very useful in many industrial applications such as printing organic electronics, but it is challenging to control the process owing to unstable flow. Here, Deblais et al.
A. Deblais +3 more
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Formation of Mn I lines in the solar atmosphere [PDF]
Astronomy & Astrophysics, 2007 We present a detailed NLTE analysis of 39 MnI lines in the solar spectrum. The influence of NLTE effects on the line formation and element abundance is investigated. Our goal is the derivation of solar log gfe values for manganese lines, which will later be used in differential abundance analysis of metal-poor stars. The method of spectrum synthesis is
Bergemann, Maria, Gehren, Thomas
openaire +2 more sources