Results 71 to 80 of about 28,742 (262)

Advancing Electronic Application of Coordination Solids: Enhancing Electron Transport and Device Integration via Surface‐Mounted MOFs (SURMOFs)

Advanced Functional Materials, Volume 36, Issue 43, 29 May 2026.
The layer‐by‐layer (LbL) assembly of coordination solids, enabled by the surface‐mounted metal‐organic framework (SURMOF) platform, is on the cusp of generating the organic counterpart of the epitaxy of inorganics. The programmable and sequential SURMOF protocol, optimized by machine learning (ML), is suited for accessing high‐quality thin films of ...
Zhengtao Xu, Christof Wöll, Stefan Bräse   +2 more
wiley   +1 more source

Very Massive Stars and Their Compact Remnants [PDF]

openAt the end of carbon burning, very massive stars (VMSs, Mstar > 100 Msun) can efficiently produce electron-positron pairs in their core, triggering an instability that leads either to the ejection of a fraction of their mass in multiple pulsations ...
SIMONATO, FILIPPO
core  

All‐in‐One Analog AI Hardware: On‐Chip Training and Inference with Conductive‐Metal‐Oxide/HfOx ReRAM Devices

Advanced Functional Materials, EarlyView.
An all‐in‐one analog AI accelerator is presented, enabling on‐chip training, weight retention, and long‐term inference acceleration. It leverages a BEOL‐integrated CMO/HfOx ReRAM array with low‐voltage operation (<1.5 V), multi‐bit capability over 32 states, low programming noise (10 nS), and near‐ideal weight transfer.
Donato Francesco Falcone, Victoria Clerico, Wooseok Choi, Tommaso Stecconi, Folkert Horst, Laura Bégon‐Lours, Matteo Galetta, Antonio La Porta, Nikhil Garg, Fabien Alibart, Bert Jan Offrein, Valeria Bragaglia   +11 more
wiley   +1 more source

X-Shooting ULLYSES: Massive Stars at Low Metallicity X. Physical Parameters and Feedback of Massive Stars in the LMC N11 B Star-Forming Region

Massive stars drive the ionization and mechanical feedback within young star-forming regions. The Large Magellanic Cloud (LMC) is an ideal galaxy for studying individual massive stars and quantifying their feedback contribution to the environment.
A. A. C. Sander, Bernini-Peron, M., Gormaz-Matamala, A.C., Kehrig, C., L. M. Oskinova, N. Morrell, D. Pauli, Todt, H., Vink, J.S., Gormaz-Matamala, A. C., O. G. Telford, A. Wofford, Shenar, T., A. Mehner, Crowther, P.A., J. S. Vink, T. Shenar, V. Ramachandran, W.-R. Hamann, Sander, A. A.C., S. R. Berlanas, van Loon, J. Th, McLeod, A. F., Telford, O. G., S. Reyero Serantes, Hamann, W. R., Mahy, L., Crowther, P. A., Kuiper, R., Vink, J. S., F. Tramper, Sander, A.C., Telford, O.G., Pauli, D., P. A. Crowther, Reyero Serantes, S., ud-Doula, A., Berlanas, S. R., H. Todt, Ramachandran, V., Leitherer, C., Tramper, F., Wofford, A., A. F. McLeod, V. M. A. Gómez-González, C. Leitherer, Gómez-González, V.M.A., Mehner, A., Oskinova, L. M., J. Th. van Loon, R. Kuiper, Gómez-González, V. M.A., Th. van Loon, J., Berlanas, S.R., Oskinova, L.M., A. ud-Doula, A. C. Gormaz-Matamala, C. Kehrig, McLeod, A.F., M. Bernini-Peron, L. Mahy, Morrell, N.   +61 more
core   +1 more source

Fundamental parameters of massive stars [PDF]

EAS Publications Series, 2004
21 pages, 3 figures, to appear in "Massive Stars: Formation, Evolution and Environment", eds. Heydari-Malayeri & Zahn (proceedings of 2002 Aussois summer school)
openaire   +2 more sources

Emergent Spin‐Glass Behavior in an Iron(II)‐Based Metal–Organic Framework Glass

Advanced Functional Materials, Volume 36, Issue 43, 29 May 2026.
A one‐pot, solvent‐free synthesis yields an Fe2+‐based metal‐organic framework (MOF) glass featuring a continuous random network structure. The material exhibits spin‐glass freezing at 14 K, driven by topological‐disorder and short‐range magnetic frustration, showcasing the potential of MOF glasses as a plattform for cooperative magnetic phenomena in ...
Chinmoy Das, Soma Salamon, Joachim Landers, Jan‐Benedikt Weiß, Wen‐Long Xue, Pascal Kolodzeiski, Roman Pallach, Heiko Wende, Sebastian Henke   +8 more
wiley   +1 more source

Division IV / Working Group on Massive Stars

, 2012
Our Working Group (WG) studies massive, luminous stars, both individually and in resolved and unresolved populations, with historical focus on early-type (OB) stars, A-supergiants, and Wolf-Rayet stars.
Leitherer, Claus, Puls, Joachim, Rauw, Grégor, Owocki, Stan, Langer, Norbert, Hanson, Margaret, Herrero, Artemio, St-Louis, Nicole, Crowther, Paul, Townsend, Richard   +9 more
core   +1 more source

IN4MER Biomaterial Ink: A Phosphorescent Biosensing Biomaterial Ink for Multiple Analytes (Glucose, Lactate, Oxygen) Measurements and Temperature Sensing Applications

Advanced Functional Materials, EarlyView.
Multianalyte, real‐time monitoring of bioprinted scaffolds remains challenging. Phosphorescence‐lifetime–based, optically responsive microparticles are embedded in diverse printable hydrogels (κ‐carrageenan, GelMA, PEGDA) to form biomaterial inks that report oxygen, glucose, lactate, and temperature.
Waqas Saleem, David Chimene, Berkley P. White, Kaivalya A. Deo, Jeremy L. Thomas, Nithin Chidambara, Cole Mandrona, Kirsten Landsgaard, Brian Ko, Roland Kaunas, Akhilesh K. Gaharwar, Michael J. McShane   +11 more
wiley   +1 more source

Massive stars with Pollux on LUVOIR

, 2019
4 pages, 3 figures, proceedings of the SF2A 2018 meetingMany open questions remain about massive stars, for example about their evolution, their wind, and their maximum mass at formation.
Bouret, J. -C., Evans, C., Neiner, C., Group, The Pollux Hot Stars Working   +3 more
core  

The Slow Merger of Massive Stars [PDF]

, 2006
We study the complete merger of two massive stars inside a common envelope and the subsequent evolution of the merger product, a rapidly rotating massive supergiant. Three qualitatively different types of mergers have been identified and investigated in detail, and the post-merger evolution has been followed to the immediate presupernova stage.
Ivanova, N, Podsiadlowski, P
openaire   +2 more sources