Results 161 to 170 of about 1,140,165 (333)
Triaxial ellipsoid dimensions and rotational pole of 2 Pallas from two stellar occultations [PDF]
J. Drummond, W. J. Cocke
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Bimetallic structures of Inconel 718 and CuCrZr are fabricated using the laser powder directed energy deposition method. The study reveals a strong dependence of interface characteristics such as width and interfusion on processing and heat treatment strategies.
Hamidreza Javidrad, Bahattin Koc
wiley +1 more source
This study focuses on stars with masses above the Kraft break in the Kepler field. Their rotational angular momenta are essentially the same as those at the zero-age main sequence.
Yu-Fu Shen+5 more
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Spectral Analysis of the Stochastic Orbits in Triaxial Stellar Systems with Figure Rotation [PDF]
Toshio Tsuchiya+2 more
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Rotary friction welding of steel E355 and the aluminum alloy EN AW‐6082 can lead to the formation of brittle intermetallic phases. The primary process parameters are varied in order to determine their influence on this intermetallic phase formation and the resulting mechanical properties.
Laura Huber+4 more
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Main-sequence broadening, Be stars, and stellar rotation inhand χ Persei [PDF]
J. Denoyelle, C. Aerts, C. Waelkens
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This study identifies 12 wt% indium (In) as the optimal composition for Sn0.5Ag0.7Cu5Bi solder joints, achieving 87% ductile fracture and 81% suppression of intermetallic compound (IMC) growth versus 4 wt% In. High‐In alloys (15–17 wt%) show abnormal IMC thickening due to thermal activation.
Liuwei Wang+11 more
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Metal-enriched Pair-instability Supernovae: Effects of Rotation
In this paper, we revisit metal-enriched rotating pair-instability supernovae (PISNe) models for metallicities consistent with the Small Magellanic Cloud, the Large Magellanic Cloud (LMC), and 0.1 Z _⊙ .
Hideyuki Umeda, Chris Nagele
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