Results 11 to 20 of about 105,284 (231)
Polyethylene (C2H4)n was compressed to pressures between 10 and 30 GPa in a diamond anvil cell (DAC) and laser heated above 2500 K for approximately one second.
E. B. Watkins+7 more
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Chemical bonding in americium oxides probed by X-ray spectroscopy
The electronic structure and the chemical state in Am binary oxides and Am-doped UO $$_2$$ 2 were studied by means of X-ray absorption spectroscopy at shallow Am core (4d and 5d) edges.
Sergei M. Butorin, David K. Shuh
doaj +1 more source
Multi-frame DVC for temporal image sequences
Digital volume correlation (DVC) is a 3D image-based technique for displacement and strain computation. Traditionally, both (digital image correlation) DIC and DVC are methods based on two individual time frames; the estimation of the displacement and ...
Zaira Manigrasso+12 more
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Gas Sloshing and Cold Fronts in Pre-merging Galaxy Cluster A98
We present deep Chandra observations of the pre-merger galaxy cluster Abell 98 (A98). A98 is a complex merging system. While the northern (A98N) and central subclusters (A98S) are merging along the north–south direction, A98S is undergoing a separate ...
Arnab Sarkar+12 more
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iid2022: a workshop on statistical methods for event data in astronomy
We review the iid2022 workshop on statistical methods for X-ray and γ-ray astronomy and high–energy astrophysics event data in astronomy, held in Guntersville, AL, on Nov. 15–18 2022.
Eric D. Feigelson+1 more
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The water dissolution mechanism in silicate melts under high pressures is not well understood. Here we present the first direct structure investigation of a water-saturated albite melt to monitor the interactions between water and the network structure ...
Robert A. Mayanovic+3 more
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The high energy X-ray probe: resolved X-ray populations in extragalactic environments
We construct simulated galaxy data sets based on the High Energy X-ray Probe (HEX-P) mission concept to demonstrate the significant advances in galaxy science that will be yielded by the HEX-P observatory.
Bret D. Lehmer+22 more
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Multiwavelength Astronomy and CTA: X-rays [PDF]
We discuss how future X-ray instruments which are under development can contribute to our understanding of the non-thermal Universe. Much progress has been made in the field of X-ray Astronomy recently, thanks to the operation of modern X-ray telescopes such as Chandra, XMM-Newton, Suzaku, and Swift, but more in-depth investigation awaits future ...
Takahashi, Tadayuki+2 more
openaire +4 more sources
Magnetic Activity–Rotation–Age–Mass Relations in Late-pre-main-sequence Stars
We study the four-dimensional relationships between magnetic activity, rotation, mass, and age for solar-type stars in the age range 5–25 Myr. This is the late-pre-main-sequence (l-PMS) evolutionary phase when rapid changes in a star's interior may lead ...
Konstantin V. Getman+2 more
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On the universal X-ray luminosity function of binary X-ray sources in galaxies [PDF]
The empirically determined universal power-law shape of X-ray luminosity function of high mass X-ray binaries in galaxies is explained by fundamental mass-luminosity and mass-radius relations for massive stars.
arxiv +1 more source