Results 111 to 120 of about 68,110 (257)

Delocalization‐ratio analysis of 3‐center bonding in position‐space for closo‐boranes and related systems: Approaching the styx picture and beyond

Journal of Computational Chemistry, Volume 45, Issue 32, Page 2862-2877, December 15, 2024.
The Wade's rules and Lipscomb's styx approach constitute a conceptual basis of chemical bonding in closo hydroborane clusters and similar compounds. Based on 3‐center electron sharing indices obtained from DFT wavefunctions, the DR approach for analysis of multicenter bonding in clusters and intermetallic compounds is presented.
Frank R. Wagner
wiley   +1 more source

MHD turbulence in the intracluster medium [PDF]

Proceedings of the International Astronomical Union, 2012
AbstractIn this work we discuss the turbulent evolution of structures in the intracluster medium based on the two fluid approximations: MHD and collisionless plasma under Chew Goldberger Low (CGL) closure. Turbulence excited by galactic motions and gas inflow in intracluster medium will develop in very different ways considering the two fluid ...
A. Lazarian, Reinaldo Santos-Lima, Diego Falceta-Gonçalves, G. Kowal, S. Nakwacki, E. M. de Gouveia Dal Pino   +5 more
openaire   +1 more source

XRISM Reveals Low Nonthermal Pressure in the Core of the Hot, Relaxed Galaxy Cluster A2029

The Astrophysical Journal Letters
We present XRISM Resolve observations of the core of the hot, relaxed galaxy cluster Abell 2029 (A2029). We find that the line-of-sight bulk velocity of the intracluster medium (ICM) within the central 180 kpc is at rest with respect to the brightest ...
XRISM Collaboration, Marc Audard, Hisamitsu Awaki, Ralf Ballhausen, Aya Bamba, Ehud Behar, Rozenn Boissay-Malaquin, Laura Brenneman, Gregory V. Brown, Lia Corrales, Elisa Costantini, Renata Cumbee, Maria Diaz Trigo, Chris Done, Tadayasu Dotani, Ken Ebisawa, Megan E. Eckart, Dominique Eckert, Satoshi Eguchi, Teruaki Enoto, Yuichiro Ezoe, Adam Foster, Ryuichi Fujimoto, Yutaka Fujita, Yasushi Fukazawa, Kotaro Fukushima, Akihiro Furuzawa, Luigi Gallo, Javier A. García, Liyi Gu, Matteo Guainazzi, Kouichi Hagino, Kenji Hamaguchi, Isamu Hatsukade, Katsuhiro Hayashi, Takayuki Hayashi, Natalie Hell, Edmund Hodges-Kluck, Ann Hornschemeier, Yuto Ichinohe, Manabu Ishida, Kumi Ishikawa, Yoshitaka Ishisaki, Jelle Kaastra, Timothy Kallman, Erin Kara, Satoru Katsuda, Yoshiaki Kanemaru, Richard Kelley, Caroline Kilbourne, Shunji Kitamoto, Shogo Kobayashi, Takayoshi Kohmura, Aya Kubota, Maurice Leutenegger, Michael Loewenstein, Yoshitomo Maeda, Maxim Markevitch, Hironori Matsumoto, Kyoko Matsushita, Dan McCammon, Brian McNamara, François Mernier, Eric D. Miller, Jon M. Miller, Ikuyuki Mitsuishi, Misaki Mizumoto, Tsunefumi Mizuno, Koji Mori, Koji Mukai, Hiroshi Murakami, Richard Mushotzky, Hiroshi Nakajima, Kazuhiro Nakazawa, Jan-Uwe Ness, Kumiko Nobukawa, Masayoshi Nobukawa, Hirofumi Noda, Hirokazu Odaka, Shoji Ogawa, Anna Ogorzalek, Takashi Okajima, Naomi Ota, Stephane Paltani, Robert Petre, Paul Plucinsky, Frederick S. Porter, Katja Pottschmidt, Kosuke Sato, Toshiki Sato, Makoto Sawada, Hiromi Seta, Megumi Shidatsu, Aurora Simionescu, Randall Smith, Hiromasa Suzuki, Andrew Szymkowiak, Hiromitsu Takahashi, Mai Takeo, Toru Tamagawa, Keisuke Tamura, Takaaki Tanaka, Atsushi Tanimoto, Makoto Tashiro, Yukikatsu Terada, Yuichi Terashima, Yohko Tsuboi, Masahiro Tsujimoto, Hiroshi Tsunemi, Takeshi Tsuru, Hiroyuki Uchida, Nagomi Uchida, Yuusuke Uchida, Hideki Uchiyama, Yoshihiro Ueda, Shinichiro Uno, Jacco Vink, Shin Watanabe, Brian J. Williams, Satoshi Yamada, Shinya Yamada, Hiroya Yamaguchi, Kazutaka Yamaoka, Noriko Yamasaki, Makoto Yamauchi, Shigeo Yamauchi, Tahir Yaqoob, Tomokage Yoneyama, Tessei Yoshida, Mihoko Yukita, Irina Zhuravleva, Tommaso Bartalesi, Stefano Ettori, Roman Kosarzycki, Lorenzo Lovisari, Tom Rose, Arnab Sarkar, Ming Sun, Prathamesh Tamhane   +138 more
doaj   +1 more source

Turbulence decay in the density-stratified intracluster medium

, 2019
Turbulence evolution in a density-stratified medium differs from that of homogeneous isotropic turbulence described by the Kolmogorov picture. We evaluate the degree of this effect in the intracluster medium (ICM) with hydrodynamical simulations. We find
Shi, Xun, Zhang, Congyao
core   +1 more source

Target Material Property‐Dependent Cluster Analysis of Inorganic Compounds

Advanced Intelligent Systems, Volume 6, Issue 12, December 2024.
A method to interpret machine learning prediction models for detecting promising material groups in terms of given material properties is developed. The developed method is validated by categorizing more than 1000 oxides into material groups, considering both basic descriptors of the composition and crystal structure and target properties such as the ...
Nobuya Sato, Akira Takahashi, Shin Kiyohara, Kei Terayama, Ryo Tamura, Fumiyasu Oba   +5 more
wiley   +1 more source

Non-thermal particles in the intergalactic and intracluster medium [PDF]

arXiv, 2004
I present a review of nonthermal processes in the large scale structure of the universe. After examining the properties of cosmological shock waves and their role as particle accelerators, I discuss the main observational facts, from radio to \gr and describe the processes that are thought be responsible for the observed nonthermal emissions.
arxiv  

The integration of circular economy and digital transformation as a catalyst for small and medium enterprise innovation

Business Strategy and the Environment, Volume 33, Issue 7, Page 7162-7181, November 2024.
Abstract This study examines the integration of digital and circular economy (CE) strategies in small and medium enterprises (SMEs) and their impact on innovation. The research uses data from the Eurobarometer survey conducted by the European Commission, which includes a sample of 16,365 SMEs.
Marta F. Arroyabe, Carlos F. A. Arranz, Juan Carlos Fernandez de Arroyabe   +2 more
wiley   +1 more source

Toward Cosmological Simulations of the Magnetized Intracluster Medium with Resolved Coulomb Collision Scale

The Astrophysical Journal
We present the first results of one extremely high-resolution, nonradiative magnetohydrodynamical cosmological zoom-in simulation of a massive cluster with a virial mass of  M _vir = 2.0 × 10 ^15 solar masses. We adopt a mass resolution of 4 × 10 ^5 M _⊙
Ulrich P. Steinwandel, Klaus Dolag, Ludwig M. Böss, Tirso Marin-Gilabert   +3 more
doaj   +1 more source

Buoyancy Instabilities in a Weakly Collisional Intracluster Medium

, 2012
The intracluster medium of galaxy clusters is a weakly collisional, high-beta plasma in which the transport of heat and momentum occurs primarily along magnetic-field lines.
Balbus, Balbus, Balbus, Bogdanović, Bogdanović, Braginskii, Cavagnolo, Christopher S. Reynolds, Dong, James M. Stone, Matthew W. Kunz, McDonald, Parrish, Parrish, Parrish, Parrish, Parrish, Parrish, Quataert, Ruszkowski, Rybicki, Sanders, Schekochihin, Schekochihin, Sharma, Sharma, Sharma, Stone, Stone, Sun, Tamara Bogdanović, Townsend, Vikhlinin, Zakamska   +33 more
core   +1 more source

Investigation of Properties of the Intercluster Medium Rich Clusters of Galaxies [PDF]

arXiv, 2010
The statistical analysis of properties of 213 rich clusters of galaxies is performed. The existence of correlations between the X-ray luminosity and the temperature of the intracluster medium and between the X-ray luminosity and the velocity dispersion of the galaxies is confirmed.
arxiv