Results 71 to 80 of about 26,905 (172)

Radio Galaxy NGC 1265 unveils the Accretion Shock onto the Perseus Galaxy Cluster

, 2011
We present a consistent 3D model for the head-tail radio galaxy NGC 1265 that explains the complex radio morphology and spectrum by a past passage of the galaxy and radio bubble through a shock wave. Using analytical solutions to the full Riemann problem
Battaglia, C. Pfrommer, Chandrasekhar, Churazov, Dursi, Dursi, Enßlin, Enßlin, Gisler, Kang, Kulsrud, Landau, Lau, Markevitch, Miley, Miniati, Quilis, Reiprich, Ryle, Ryu, Ryu, Ryu, Sijbring, Sun, T. W. Jones, Tremaine   +25 more
core   +1 more source

A Shock-Induced Pair of Superbubbles in the High-Redshift Powerful Radio Galaxy MRC 0406-244 [PDF]

, 2001
We present new optical spectroscopy of the high-redshift powerful radio galaxy MRC 0406$-$244 at redshift of 2.429. We find that the two extensions toward NW and SE probed in the rest-frame ultraviolet image are heated mainly by the nonthermal continuum ...
Alexander P. A., Arimoto N., Best P. N., De Breuck C., George Kosugi, Hiroko Taguchi, Hiroshi Sudou, Kazuhiro Sekiguchi, Kentaro Aoki, Kiichi Okita, Koji S. Kawabata, Masanori Iye, Masaru Ajiki, Michitoshi Yoshida, Motohara K., Motoko Inata, Noboru Ebizuka, Nobunari Kashikawa, Rees M. J., Rie R. Kobayashi, Rottgering H. J. A., Saeko Noda, Scarrott S. M., Shingo Nishiura, Shinobu S. Fujita, Tadafumi Takata, Takashi Murayama, Tohru Nagao, Tomohiko Ozawa, Toshiyuki Sasaki, Villar-Martin M., Yasuhiro Shimizu, Yasuhiro Shioya, Yasushi Yadomaru, Yohei Koyama, Yoshiaki Taniguchi, Yoshihiko Saito, Youichi Ohyama, Yuko Kakazu   +38 more
core   +2 more sources

GOES‐R Series X‐Ray Sensor (XRS): 2. On‐Orbit Measurements and Calibrations

Journal of Geophysical Research: Space Physics, Volume 131, Issue 5, May 2026.
Abstract An X‐Ray Sensor (XRS) has been onboard each of the National Oceanic and Atmospheric Administration (NOAA) Geostationary Operational Environmental Satellites (GOES) since 1975. XRS measures full‐disk soft X‐ray irradiance in two wavelength bands, 0.05–0.4 nm and 0.1–0.8 nm.
Janet L. Machol, Stefan M. Codrescu, Courtney L. Peck, Elysia S. Lucas, James F. Mothersbaugh III, Thomas N. Woods, Ann Marie Mahon, James Negus, Donald L. Woodraska, Thomas D. Eden Jr., Francis G. Eparvier, Andrew R. Jones, Brooke Kotten, Laurel A. Rachmeler, Andrew C. Wilson, Brian T. Kress, Juan V. Rodriguez, Rodney A. Viereck   +17 more
wiley   +1 more source

A Possible Solution to the Mystery of the ANITA Anomalous Events

Annalen der Physik, Volume 538, Issue 4, April 2026.
In 2006 and 2014, the Antarctic Impulsive Transient Antenna (ANITA), a balloon‐borne radio observatory flying over Antarctica, detected two strange upward‐going radio pulse events that have not yet been explained by our current understanding of physics.
Massimo Villata
wiley   +1 more source

Mapping the particle acceleration in the cool core of the galaxy cluster RX J1720.1+2638

, 2014
We present new deep, high-resolution radio images of the diffuse minihalo in the cool core of the galaxy cluster RX J1720.1+2638. The images have been obtained with the Giant Metrewave Radio Telescope at 317, 617 and 1280 MHz and with the Very Large ...
Bourdin, Hervé, Brunetti, Gianfranco, Giacintucci, Simona, Markevitch, Maxim, Mazzotta, Pasquale, Venturi, Tiziana, ZuHone, John A.   +6 more
core   +1 more source

A diffuse bubble-like radio-halo source MRC 0116+111: imprint of AGN feedback in a low-mass cluster of galaxies [PDF]

, 2009
We present detailed observations of MRC 0116+111, revealing a luminous, mini radio-halo of ~240 kpc diameter located at the centre of a cluster of galaxies at redshift z = 0.131.
A. C. Kumbharkhane, Aharonian, Allen, Baars, Bagchi, Bagchi, Becker, Begelman, Binney, Birzan, Birzan, Blanton, Brunetti, Brüggen, Brüggen, Burns, Böhringer, Canizares, Cassano, Cattaneo, Churazov, Churazov, Cohen, Colafrancesco, Condon, Dalla Vecchia, De Young, Dunn, Dunn, Edge, Ensslin, Ensslin, Fabian, Fabian, Fabian, Fabian, Feretti, Ferrari, Ghizzardi, Giovannini, Gitti, Gitti, Gitti, Gopal-Krishna, Gopal-Krishna, , Govoni, Gull, Harms, Heckman, Hinton, Jamrozy, Jaydeep Belapure, Joe Jacob, Joshi, Joydeep Bagchi, Landolt, Large, Loeb, Lopes, McNamara, McNamara, McNamara, McNamara, McNamara, Mittal, Murgia, Nitin Wadnerkar, Norbert Werner, Owen, Parma, Pedlar, Peterson, Pfrommer, Rafferty, Reiprich, Ruszkowski, Ryu, Salome, Sanders, Slee, Soker, Stanek, Swarup, Venturi, Völk, Wise   +85 more
core   +2 more sources

Understanding Degradation Mechanisms in Water‐In‐Salt Electrolyte. Part 2: Impact of the Electrochemical Parameters on the Cycling Behavior of LiFePO4 versus TiS2

Batteries &Supercaps, Volume 9, Issue 4, April 2026.
Cycling water‐in‐salt batteries involves complex degradation processes that require multiprobe analysis. Using online electrochemical mass spectrometry (OEMS), postmortem X‐ray photoemission spectroscopy (XPS) (including hard‐XPS), and scanning electron microscopy (SEM), the degradation mechanisms are examined in composite electrodes (TiS2 and LiFePO4)
Célia Doublet, Théo Faverge, Vincent Martin, Hiram Castillo Michel, Jean‐Pascal Rueff, Marian Chatenet, Lauréline Lecarme, Claire Villevieille   +7 more
wiley   +1 more source

Black hole masses and starbursts in X-shaped radio sources

, 2011
It has been suggested that the X-shaped morphology observed in some radio sources can reflect either a recent merger of two supermassive black holes (SMBHs) or the presence of a second active black hole in the galactic nucleus. These scenarios are tested
A. P. Lobanov, Adelman-McCarthy, Antonucci, Asari, Becker, Bruzual, Capetti, Cardelli, Cheung, Cheung, Cid Fernandes, Cid Fernandes, Cid Fernandes, de Vries, Dennett-Thorpe, Dokuchaev, Efstathiou, Frenk, Gebhardt, Gergely, González-Serrano, Gopal-Krishna, Biermann, Hodges-Kluck, Hodges-Kluck, Hopkins, Hutchings, Hutchings, J. León-Tavares, Kaspi, Kaspi, Lal, Lal, Landt, Landt, Leahy, Lobanov, M. Mezcua, Mack, Marcha, Marchesini, Mateus, Merritt, Merritt, Nelson, Parma, Plotkin, Rees, Sanders, Schlegel, Stocke, Strateva, Tingay, Toomre, Tremaine, V. H. Chavushyan, Wang, Wu   +56 more
core   +1 more source

Engineering Asymmetry: How Chirality Boosts Catalysis, Spin Selectivity, and Light–Matter Interactions

ChemPhotoChem, Volume 10, Issue 4, April 2026.
This review connects chiroptical spectroscopy, asymmetric catalysis, and spintronics, revealing how chirality influences the interactions of matter with light, charge, and spin. Across diverse systems, remarkable chiroptical effects emerge, showing among others that high efficiencies can arise without absolute enantiopurity, and that functionality is ...
Charitini Panagiotopoulou, Maedeh Anisi, Changseop Jeong, Kamyar Shameli, J. Lorenzo Alonso‐Gómez, Aras Kartouzian   +5 more
wiley   +1 more source

Magnetic Fields in the Milky Way and in Galaxies

, 2018
Most of the visible matter in the Universe is ionized, so that cosmic magnetic fields are quite easy to generate and due to the lack of magnetic monopoles hard to destroy. Magnetic fields have been measured in or around practically all celestial objects,
Beck, Rainer, Wielebinski, Richard
core   +1 more source