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Mostrando 861 - 880 Resultados de 912 Para Buscar '"stellarator"', tiempo de consulta: 0.12s Limitar resultados
  1. 861
    “…By including radiation loss with post-Newtonian techniques, we evolve stellar-mass secondary objects around a supermassive Zipoy-Voorhees primary and find clear imprints of non-integrability in these systems. …”
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    Geodesics and gravitational waves in chaotic extreme-mass-ratio inspirals: the curious case of Zipoy-Voorhees black-hole mimickers
  2. 862
    “…Based on the reported results, a photon-counting detector CT arthrography of the ankle with an ultra-high-resolution collimation offers stellar image quality and tissue assessability, improving the evaluation of miniscule anatomical structures. …”
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    Ultra-High-Resolution Photon-Counting Detector CT Arthrography of the Ankle: A Feasibility Study
  3. 863
    por Jhade, D, Ahirwar, D, Jain, R, Sharma, NK, Gupta, S
    Publicado 2011
    “…Microscopically, the root showed cork, cortex, stellar region, and calcium oxalate crystals. Powder microscopy showed anamalous secondary growth in between the xylem vessels and Calcium Oxalate crystals in the cortex region. …”
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    Pharmacognostic Standardization, Physico- and Phytochemical Evaluation of Amaranthus Spinosus Linn. Root
  4. 864
    “…Owing to the close distance to Orion (about 1,350 light-year), the effects of stellar feedback on the parental cloud can be studied in detail. …”
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    Compression and ablation of the photo-irradiated molecular cloud the Orion Bar
  5. 865
    por Toriumi, Shin, Wang, Haimin
    Publicado 2019
    “…Finally, we discuss the outstanding issues and future perspective and further broaden our scope to the possible applications of our knowledge to space-weather forecasting, extreme events in history, and corresponding stellar activities. ELECTRONIC SUPPLEMENTARY MATERIAL: The online version of this article (10.1007/s41116-019-0019-7) contains supplementary material, which is available to authorized users.…”
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    Flare-productive active regions
  6. 866
    “…The essentiality of Nit11764 for cyanotrophy remains uncertain given that cyanide itself is a poor substrate and the catalytic efficiencies for even the best of nitrile substrates (~5 × 10(3) M(−1) s(−1)) is less than stellar.…”
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    Characterization of the Nit6803 nitrilase homolog from the cyanotroph Pseudomonas fluorescens NCIMB 11764
  7. 867
    por Wasowicz, Tomasz J.
    Publicado 2021
    “…In particular, the investigations on bond-breaking and new bond-forming processes triggered by the ionic impact may shed light on the stellar wind interaction with interstellar media, ionic beam irradiations of the living cells, ion-track nanotechnology, radiation hardness analysis of materials, and focused ion beam etching, deposition, and lithography. …”
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    Neutral Dissociation of Pyridine Evoked by Irradiation of Ionized Atomic and Molecular Hydrogen Beams
  8. 868
    “…The temperatures and turbulent velocities do not show significant trends with stellar distance or angle from the LIC center. If/when the Sun enters an inter-cloud medium, the physical properties of the future heliosphere will be very different from the present. …”
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    Inhomogeneity in the Local ISM and Its Relation to the Heliosphere
  9. 869
    “…Impactful academic research plays a stellar role in society, pressing to ask the question of how one measures the impact created by different areas of academic research. …”
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    Measuring the Impact of Research: Lessons from the UK’s Research Excellence Framework 2014
  10. 870
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    Pharmacokinetics and distribution of 2‐hydroxypropyl‐β‐cyclodextrin following a single intrathecal dose to cats
  11. 871
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    Electrographic Features of Spontaneous Recurrent Seizures in a Mouse Model of Extended Hippocampal Kindling
  12. 872
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    A scoping review to inform a multi-disciplinary approach for nutrition therapy in critically ill children with pressure injuries
  13. 873
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    Turning toward or away from God: COVID-19 and changes in religious devotion
  14. 874
    por Guerrero, C, Lerendegui-Marco, J, Paul, M, Tessler, M, Heinitz, S, Domingo-Pardo, C, Cristallo, S, Dressler, R, Halfon, S, Kivel, N, Köster, U, Maugeri, E A, Palchan-Hazan, T, Quesada, J M, Rochman, D, Schumann, D, Weissman, L, Aberle, O, Amaducci, S, Andrzejewski, J, Audouin, L, Bécares, V, Bacak, M, Balibrea, J, Barak, A, Barbagallo, M, Barros, S, Bečvář, F, Beinrucker, C, Berkovits, D, Berthoumieux, E, Billowes, J, Bosnar, D, Brugger, M, Buzaglo, Y, Caamaño, M, Calviño, F, Calviani, M, Cano-Ott, D, Cardella, R, Casanovas, A, Castelluccio, D M, Cerutti, F, Chen, Y H, Chiaveri, E, Colonna, N, Cortés, G, Cortés-Giraldo, M A, Cosentino, L, Dafna, H, Damone, A, Diakaki, M, Dietz, M, Dupont, E, Durán, I, Eisen, Y, Fernández-Domínguez, B, Ferrari, A, Ferreira, P, Finocchiaro, P, Furman, V, Göbel, K, García, A R, Gawlik, A, Glodariu, T, Gonçalves, I F, González-Romero, E, Goverdovski, A, Griesmayer, E, Gunsing, F, Harada, H, Heftrich, T, Heyse, J, Hirsh, T, Jenkins, D G, Jericha, E, Käppeler, F, Kadi, Y, Kaizer, B, Katabuchi, T, Kavrigin, P, Ketlerov, V, Khryachkov, V, Kijel, D, Kimura, A, Kokkoris, M, Kriesel, A, Krtička, M, Leal-Cidoncha, E, Lederer-Woods, C, Leeb, H, Lo Meo, S, Lonsdale, S J, Losito, R, Macina, D, Manna, A, Marganiec, J, Martínez, T, Massimi, C, Mastinu, P, Mastromarco, M, Matteucci, F, Mendoza, E, Mengoni, A, Milazzo, P M, Millán-Callado, M A, Mingrone, F, Mirea, M, Montesano, S, Musumarra, A, Nolte, R, Oprea, A, Patronis, N, Pavlik, A, Perkowski, J, Piersanti, L, Porras, I, Praena, J, Rajeev, K, Rauscher, T, Reifarth, R, Rodríguez-González, T, Rout, P C, Rubbia, C, Ryan, J A, Sabaté-Gilarte, M, Saxena, A, Schillebeeckx, P, Schmidt, S, Shor, A, Sedyshev, P, Smith, A G, Stamatopoulos, A, Tagliente, G, Tain, J L, Tarifeño-Saldivia, A, Tassan-Got, L, Tsinganis, A, Valenta, S, Vannini, G, Variale, V, Vaz, P, Ventura, A, Vlachoudis, V, Vlastou, R, Wallner, A, Warren, S, Weigand, M, Weiss, C, Wolf, C, Woods, P J, Wright, T, Žugec, P
    Publicado 2020
    “…The neutron capture cross sections of several unstable nuclides acting as branching points in the s process are crucial for stellar nucleosynthesis studies. The unstable Tm171 (t1/2=1.92  yr) is part of the branching around mass A∼170 but its neutron capture cross section as a function of the neutron energy is not known to date. …”
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    Neutron Capture on the $s$-Process Branching Point $^{171}$Tm via Time-of-Flight and Activation
  15. 875
    “…Our results confirm recent predictions of radiation belts at both ends of the stellar mass sequence(8,16–19) and support broader re-examination of rotating magnetic dipoles in producing non-thermal quiescent radio emissions from brown dwarfs(7), fully convective M dwarfs(20) and massive stars(18,21).…”
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    Resolved imaging confirms a radiation belt around an ultracool dwarf
  16. 876
    “…Many stellar configurations, including white dwarfs, neutron stars, black holes, supermassive stars, and star clusters, rely on relativistic effects. …”
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    Analysis of the fractional relativistic polytropic gas sphere
  17. 877
    por Davis, Christopher Sean
    Publicado 2016
    “…Near the equator, solar and stellar horizon sightings most visibly track the passage of time and seasonal cycles. …”
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    Solar-Aligned Pictographs at the Paleoindian Site of Painel do Pilão along the Lower Amazon River at Monte Alegre, Brazil
  18. 878
    “…In the present study, we used these ISS imaging results, together with ultraviolet imaging spectrograph stellar and solar occultation measurements and modeling of the three-dimensional structure of the vapor cloud, to constrain the magnitudes, velocities, and time variability of the plume gas sources from the INMS data. …”
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    Enceladus Plume Structure and Time Variability: Comparison of Cassini Observations
  19. 879
    “…Observations have previously shown that interactions between multiple members, including a high-speed intruder galaxy currently colliding into the intragroup medium, have probably generated tidal debris in the form of multiple gaseous and stellar filaments(6,8,13), the formation of tidal dwarfs(7,14,15) and intragroup-medium starbursts(16), as well as widespread intergalactic shocked gas(5,10,11,17). …”
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    A 0.6 Mpc H i structure associated with Stephan’s Quintet
  20. 880
    por Ghez, Andrea
    Publicado 2020
    “…After more than a decade of diffraction-limited imaging on large ground-based telescopes, the case for a supermassive black hole at the Galactic center has gone from a possibility to a certainty, thanks to measurements of individual stellar orbits. The rapidity with which these stars move on small-scale orbits indicates a source of tremendous gravity and provides the best evidence that supermassive black holes, which confront and challenge our knowledge of fundamental physics, do exist in the Universe. …”
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    Our Galactic Center: A Unique Laboratory for the Physics & Astrophysics of Black Holes
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