Results 271 to 280 of about 1,250,237 (300)

Au₂₀Ag₃₂ Nanocluster Emitting Bright Near-Infrared-II Photoluminescence with Quantum Yield of 30% in Aerated Solution. [PDF]

ACS Nano
Sardar A, Wang Y, He G, Gianopoulos CG, Samarasinghe DSND, Liu Z, Kirschbaum K, Aikens CM, Jin R.   +8 more
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Hidden Stacking Fault Charge Traps in Hexagonal Boron Nitride and Their Impact on Dielectric Breakdown. [PDF]

Nano Lett
Lang T, Liu Y, Chugh A, Watanabe K, Taniguchi T, Lee HY.   +5 more
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Radiative Defects in Chloride-Activated CdSe Thin Films. [PDF]

ACS Energy Lett
Abudulimu A, Wang X, Brau T, Kuliček J, Wenner SL, Phillips AB, Bastola E, Jamarkattel MK, Karade VC, Lamichhane K, Dixit A, Rezek B, Yan Y, Heben MJ, Ellingson RJ.   +14 more
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Development of hybrid nanoparticles based on Zr(iv) and perylene-3,4,9,10-tetracarboxylic acid with visible-light photoredox activity. [PDF]

RSC Adv
Cacciari RD, Gonik E, Beltrán AM, Mizrahi MD, Ezquerra Riega SD, Rodríguez HB, Gonzalez MC.   +6 more
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Correction for Herpe et al., When alternative becomes essential: The role of mitochondrial glycerol-3-phosphate dehydrogenase. [PDF]

Proc Natl Acad Sci U S A
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Broad emission lines in active galactic nuclei. I - an atlas of H-alpha and H-beta profiles

, 1990
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Variation of the Hβ Emission Lines of YY Geminorum

Publications of the Astronomical Society of Japan, 1980
Abstract Forty-four image-tube spectra of YY Gem (4 Å mm−1, λλ 4820–4900 Å) are analyzed to yield the radial velocity curves and the variations in the intensity and the width of Hβ emission lines during the quiescent phase at epoch 1978 January 4–8. The present study disagrees with the claim by Leung and Schneider (1978) that the orbital
Keiichi Kodaira, Kihachiro Ichimura
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Observation of enhanced emission of the O VIII Hα line in a recombining laser-produced plasma

Applied Physics Letters, 1984
We have observed enhanced emission of the O VIII Hα line at 121 eV from a recombining plasma produced by laser heating of a thin Formvar foil with two opposed cylindrically focused (0.3×1.4 cm) 5-TW laser beams. The time-dependent intensity of the Hα line increases by nearly an order of magnitude as the plasma length is increased from 0.27 to 1.27 cm ...
D. L. Matthews, E. M. Campbell, K. Estabrook, W. Hatcher, R. L. Kauffman, R. W. Lee, C. L. Wang   +6 more
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Variation of the Hβ Emission Lines of YY Geminorum. II. Change of Sectorial Structures of Active Regions

Publications of the Astronomical Society of Japan, 1982
Abstract Sixty-three image-tube spectrograms of YY Gem (4 Å mm−1, λλ4820–4900 Å) are analyzed to yield the radial-velocity curves and the variations in the intensities and the widths of Hβ emission lines during the quiescent phase at epochs 1980 February 11–16, 1981 January 14–15, and 1981 March 11.
Keiichi Kodaira, Kihachiro Ichimura
openaire   +1 more source