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801por Kowalska, Magdalena“…They also contribute to our understanding of the stellar nucleosynthesis. </span></span></span></p> <p><span><span><span>This talk will concentrate on two probably less know aspects of ISOLDE research: Beyond Standard Model studies and life science applications. …”
Publicado 2021
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802por Banks, Hannah Molly“…Crucially we will find that the inspiral phases of stellar-mass compact binary systems cumulatively produce a signal well within reach of the proposed AION-km and AEDGE experiments. …”
Publicado 2023
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803por Fields, Brian“… We will summarize possible resolutions to this "lithium problem," highlighting recent work that strengthens the case for a a solution involving stellar astrophysics, while solutions involving new physics are becoming ever more constrained. …”
Publicado 2023
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804“…We identify numerous constraints on any such scenario, ultimately concluding that observable effects on the dynamics of binary inspirals due to such a force are not possible if the dark matter is accrued during ordinary stellar evolution. Constraints arise from the requirement that the astronomical body be able to collect and bind at small enough radius an adequate number of dark matter particles, from the requirement that the particles thus collected remain bound to neutron stars in the presence of another neutron star, and from the requirement that the theory allows old neutron stars to exist and retain their charge. …”
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805por Babiano-Suarez, V, Caballero, L, Domingo-Pardo, C, Ladarescu, I, Aberle, O, Alcayne, V, Amaducci, S, Andrzejewski, J, Audouin, L, Bacak, M, Barbagallo, M, Bécares, V, Bečvář, F, Bellia, G, Berthoumieux, E, Billowes, J, Bosnar, D, Brown, A S, Busso, M, Caamaño, M, Calviani, M, Calviño, F, Cano-Ott, D, Casanovas, A, Cerutti, F, Chen, Y H, Chiaveri, E, Colonna, N, Cortés, G P, Cortés-Giraldo, M A, Cosentino, L, Cristallo, S, Damone, L A, Diakaki, M, Dietz, M, Dressler, R, Dupont, E, Durán, I, Eleme, Z, Fernández-Domíngez, B, Ferrari, A, Ferro-Gon calves, I, Finocchiaro, P, Furman, V, Gawlik, A, Gilardoni, S, Glodariu, T, Göbel, K, González-Romero, E, Guerrero, C, Gunsing, F, Heinitz, S, Heyse, J, Jenkins, D G, Kadi, Y, Käppeler, F, Kimura, A, Kivel, N, Kokkoris, M, Kopatch, Y, Krtička, M, Kurtulgil, D, Lederer-Woods, C, Lerendegui-Marco, J, Lo Meo, S, Lonsdale, S J, Macina, D, Manna, A, Martínez, T, Masi, A, Massimi, C, Mastinu, P F, Mastromarco, M, Matteucci, F, Maugeri, E, Mazzone, A, Mendoza, E, Mengoni, A, Michalopoulou, V, Milazzo, P M, Mingrone, F, Musumarra, A, Negret, A, Nolte, R, Ogállar, F, Oprea, A, Patronis, N, Pavlik, A, Perkowski, J, Piersanti, L, Porras, I, Praena, J, Quesada, J M, Radeck, D, Ramos Doval, D, Rausher, T, Reifarth, R, Rochman, D, Rubbia, C, Sabaté-Gilarte, M, Saxena, A, Schillebeeckx, P, Schumann, D, Smith, A G, Sosnin, N, Stamatopoulos, A, Tagliente, G, Tain, J L, Talip, Z, Tarifeño-Saldivia, A E, Tassan-Got, L, Tsinganis, A, Ulrich, J, Urlass, S, Valenta, S, Vannini, G, Variale, V, Vaz, P, Ventura, A, Vlachoudis, V, Vlastou, R, Wallner, A, Woods, P J, Wright, T J, Žugec, P“…Such system is being developed at the “Gamma Spectroscopy and Neutrons Group” at IFIC ( http://webgamma.ific.uv.es/gamma/es/ , [2]), in the framework of the ERC-funded project HYMNS (High sensitivitY and Measurements of key stellar Nucleo-Synthesis reactions). This work summarizes first tests with neutron beam at CERN n $\_$ TOF.…”
Publicado 2019
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806por Margerin, V, Murphy, A St J, Davinson, T, Dressler, R, Fallis, J, Kankainen, A, Laird, A M, Lotay, G, Mountford, D J, Murphy, C D, Seiffert, C, Schumann, D, Stowasser, T, Stora, T, Wang, C H -T, Woods, P J“…Conveniently, the amount of this isotope in stellar ejecta is thought to depend critically on the explosion mechanism. …”
Publicado 2014
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807por Oprea, Cristiana, Mihul, Alexandru, Oprea, Alexandru Ioan, Zgura, Sorin, Potlog, Mihai, Neagu, Alina“…Due to the high temperature and large densities of gamma quanta, neutrons and protons in stellar environment $^{146} \mathrm{Sm}$ nucleus can be obtained in (γ,n), (n,2n), (p,2n) processes on $^{146} \mathrm{Sm}$ .The knowledge of corresponding cross sections of gamma rays, neutrons and alpha induced processes is of a great importance for the explanation of ($^{146} \mathrm{Sm}$ /$^{144} \mathrm{Sm}$ ) ratio uncertainties observed on the Earth, meteorites, Moon and other celestial bodies.Cross sections of (γ,n), (n,2n), (α,γ) processes induced by fast gamma rays, neutrons and alphas on $^{147} \mathrm{Sm}$ and $^{142} \mathrm{Nd}$ from threshold up to 25 MeV were evaluated and predicted in the frame of Hauser-Feshbach statistical model by using Talys software and the own computer programs. …”
Publicado 2020
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808por Pontigo, Sofía, Parra-Almuna, Leyla, Luengo-Escobar, Ana, Poblete-Grant, Patricia, Nunes-Nesi, Adriano, Mora, María de la Luz, Cartes, Paula“…Accordingly, two cultivars with high PAE but low PUE (Ansa and Stellar), and two cultivars with low PAE and high PUE (24Seven and Extreme) were selected to analyze the activity and gene expression of acid phosphatases (APases), as well as the transcript levels of P transporters. …”
Publicado 2023
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809“…After which we examine three scenarios: (1) the determination of the location and magnitude of multiple point charges through a single observation, (2) the learning of electrical and mechanical sensor properties and the characteristics of an electrical field through several observations, (3) the possibility that an observer can infer their location and orientation in a fixed and known electrical field (akin to “stellar navigation”). To conclude, we discuss the potential of electroreception to endow an animal with thus far unappreciated sensory capabilities, such as the mapping of electrical environments. …”
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810por Migliorini, Filippo, Maffulli, Nicola, Schäfer, Luise, Schneider, Jens, Nobili, Andrea Maria, Kämmer, Daniel, Michalak, Milosch, Bell, Andreas“…A restricted kinematic alignment with medial para-stellar approach shall be made in all patients. The present study follows the SPIRIT guidelines. …”
Publicado 2023
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811por Burbach, J. Peter H., Grant, Philip, Hellemons, Anita J. C. G. M., Degiorgis, Joseph A., Li, Ka Wan, Pant, Harish C.“…Intense staining for FMRFamide in the adult SG was confined to microneurons and fibers in the neuropil and to small fibers surrounding giant axons in stellar nerves. This shows that the Fmrf gene in the SG is strongly regulated post-hatching, and suggests that the FMRFamide precursor is incompletely processed in the adult SG. …”
Publicado 2013
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812por Ramirez, Ramses M.“…Similar extensions are shown for stars with stellar effective temperatures between 2,600–9,000 K. …”
Publicado 2020
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813“…Instead, for typical stellar-mass black holes, [Formula: see text] may drop well below [Formula: see text]. …”
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814por Jiang, Linyi, Li, Xiaoyan, Li, Liyuan, Yang, Lin, Yang, Lan, Hu, Zhuoyue, Chen, Fansheng“…Then, we analyze the relative motion transformation of the observed stars. The stellar trajectory and the auxiliary ephemeris are used to obtain the corresponding object vector for correcting the associated calibration parameters iteratively. …”
Publicado 2021
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815por Baum, Seth D.“…The paper analyzes natural climate change, natural pandemics, near-Earth objects (asteroids, comets, and meteors), space weather (coronal mass ejections, solar flares, and solar particle events), stellar explosions (gamma-ray bursts and supernovae), and volcanic eruptions. …”
Publicado 2022
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816“…However, there are also issues in interpreting the stellar materials and reproducing their high ionic conductivities. …”
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817por Beskin, Vasily S“…Finally, on the basis of the full MHD version of the Grad-Shafranov equation the author discusses the problems of jet collimation and particle acceleration in Active Galactic Nuclei, radio pulsars, and Young Stellar Objects. The comparison of the analytical results with numerical simulations demonstrates their good agreement. …”
Publicado 2010
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818“…Close Binaries are classic examples of the fundamental contribution that stellar astrophysics makes to our general understanding of physical processes in the universe. …”
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819“…This book provides detailed descriptions of the ten known systems, illustrates them richly with examples of new spectra, and places them in the context of stellar structure and evolution. Comprised of a large cool giant plus a small hot dwarf, these key eclipsing binaries reveal fascinating changes in their spectra very close to total eclipse, when the hot star shines through differing heights of the "chromosphere", or outer atmosphere, of the giant star. …”
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820“…Use of occultation methodology for observing the Earth's atmosphere and climate has become so broad as to comprise solar, lunar, stellar, navigation and satellite crosslink occultation methods. …”
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