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  1. 441
    por Casanovas, A, Tarifeño-Saldivia, A E, Domingo-Pardo, C, Calviño, F, Maugeri, E, Guerrero, C, Lerendegui-Marco, J, Dressler, R, Heinitz, S, Schumann, D, Tain, J L, Quesada, J M, Aberle, O, Alcayne, V, Amaducci, S, Andrzejewski, J, Audouin, L, Babiano-Suarez, V, Bacak, M, Balibrea, J, Barbagallo, M, Bennett, S, Berthoumieux, E, Bosnar, D, Brown, A S, Busso, M, Caamaño, M, Caballero, L, Calviani, M, Cano-Ott, D, Cerutti, F, Chiaveri, E, Colonna, N, Cortés, G P, Cortés-Giraldo, M A, Cosentino, L, Cristallo, S, Damone, L A, Davies, P J, Diakaki, M, Dietz, M, Ducasse, Q, Dupont, E, Durán, I, Eleme, Z, Fernández-Domíngez, B, Ferrari, A, Ferro-Gonçalves, I, Finocchiaro, P, Furman, V, Garg, R, Gawlik, A, Gilardoni, S, Göbel, K, González-Romero, E, Gunsing, F, Heyse, J, Jenkins, D G, Jericha, E, Jiri, U, Junghans, A, Kadi, Y, Käppeler, F, Kimura, A, Knapová, I, Kokkoris, M, Kopatch, Y, Krticka, M, Kurtulgil, D, Ladarescu, I, Lederer-Woods, C, Lonsdale, S J, Macina, D, Manna, A, Martínez, T, Masi, A, Massimi, C, Mastinu, P F, Mastromarco, M, Mazzone, A, Mendoza, E, Mengoni, A, Michalopoulou, V, Milazzo, P M, Millán-Callado, M A, Mingrone, F, Moreno-Soto, J, Musumarra, A, Negret, A, Ogállar, F, Oprea, A, Patronis, N, Pavlik, A, Perkowski, J, Petrone, C, Piersanti, L, Pirovano, E, Porras, I, Praena, J, Ramos Doval, D, Reifarth, R, Rochman, D, Rubbia, C, Sabaté-Gilarte, M, Saxena, A, Schillebeeckx, P, Sekhar, A, Smith, A G, Sosnin, N, Sprung, P, Stamatopoulos, A, Tagliente, G, Tassan-Got, L, Thomas, B, Torres-Sánchez, P, Tsinganis, A, Urlass, S, Valenta, S, Vannini, G, Variale, V, Vaz, P, Ventura, A, Vescovi, D, Vlachoudis, V, Vlastou, R, Wallner, A, Woods, P J, Wright, T J, Žugec, P, Koester, U
    Publicado 2020
    “…At some particular stellar s-process environments, the decay of both nuclei is strongly enhanced, and determines decisively the abundance of two s-only isotopes of lead, $^{204} \mathrm{Pb}$ and $^{205} \mathrm{Pb}$. …”
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    Neutron capture measurement at the n TOF facility of the $^{204}$Tl and $^{205}$Tl s-process branching points
  2. 442
    “…Phosphorus-rich stars likely inherit their peculiar chemistry from another nearby stellar source but their intriguing chemical abundance pattern challenge the present stellar nucleosynthesis theoretical predictions. …”
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    Phosphorus-rich stars with unusual abundances are challenging theoretical predictions
  3. 443
    “…We integrate the semiclassical equations of (spherically symmetric) stellar equilibrium for a constant-density classical fluid. …”
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    Semiclassical relativistic stars
  4. 444
    “…There was a further reduction after the implementation of stellar detectors reflected in a reduction of 36% of the dose–length product for thoracic scans. …”
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    Evaluating the effect of increased pitch, iterative reconstruction and dual source CT on dose reduction and image quality
  5. 445
    por Lebedev, Sergey V
    Publicado 2007
    “…Every two years, at the International conference on High Energy Density Laboratory Astrophysics, scientists interested in this emerging field discuss the progress in topics covering: - Stellar evolution, stellar envelopes, opacities, radiation transport - Planetary Interiors, high-pressure EOS, dense plasma atomic physics - Supernovae, gamma-ray bursts, exploding systems, strong shocks, turbulent mixing - Supernova remnants, shock processing, radiative shocks - Astrophysical jets, high-Mach-number flows, magnetized radiative jets, magnetic reconnection - Compact object accretion disks, x-ray photoionized plasmas - Ultrastrong fields, particle acceleration, collisionless shocks. …”
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    High Energy Density Laboratory Astrophysics
  6. 446
    por Gershberg, Roald E
    Publicado 2005
    “…The analysis of the various manifestations of such stellar activity leads to the identification of these phenomena with macroscopic non-linear processes in a magnetized plasma. …”
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    Solar-Type Activity in Main-Sequence Stars
  7. 447
    por Matteucci, Francesca
    Publicado 2012
    “…This book deals with the chemical evolution of galaxies of all morphological types (ellipticals, spirals and irregulars) and stresses the importance of the star formation histories in determining the properties of stellar populations in different galaxies. The topic is approached in a didactical and logical manner via galaxy evolution models which are compared with observational results obtained in the last two decades: The reader is given an introduction to the concept of chemical abundances and learns about the main stellar populations in our Galaxy as well as about the classification of galaxy types and their main observables. …”
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    Chemical evolution of galaxies
  8. 448
    por Mobberley, Martin
    Publicado 2007
    “…Supernovae represent the most violent stellar explosions in the universe. This book presents supernovo facts and explains what they are, and how to observe and discover them. …”
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    Supernovae and how to observe them
  9. 449
    Publicado 2002
    “…Paul Davies has analysed light from some of the most distant stellar objects in the sky. From these observations he has concluded that the speed of light was faster billions of years ago than it is today (1/2 page).…”
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    Relative values: shedding light on Einstein's theories
  10. 450
    por Meadows, A. J. (Arthur Jack)
    Publicado 1986
    Libro
    Evolución estelar /
  11. 451
    “…The extreme luminosities of massive, hot OB stars drive strong stellar winds through line-scattering of the star's UV continuum radiation. …”
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    Line-driven ablation of circumstellar discs – I. Optically thin decretion discs of classical Oe/Be stars
  12. 452
    “…Although still unresolved, stellar UV circularly polarized light (CPL) is the leading hypothesis to have caused the symmetry breaking in space. …”
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    Uncovering the chiral bias of meteoritic isovaline through asymmetric photochemistry
  13. 453
    “…Complex disordered matter is of central importance to a wide range of disciplines, from bacterial colonies and embryonic tissues in biology to foams and granular media in materials science to stellar configurations in astrophysics. Because of the vast differences in composition and scale, comparing structural features across such disparate systems remains challenging. …”
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    Topological packing statistics of living and nonliving matter
  14. 454
    por Shore, S N, Livio, M, van den Heuvel, EPJ
    Publicado 1994
    “…The contributors deal with symbiotic stars, cataclysmic variables, massive binaries and X-ray binaries, in an attempt to provide a better understanding of stellar evolution.…”
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    Interacting binaries
  15. 455
    “…Our analysis indicates that a clear, novel, and observable, coronal response is generated due to the collapse of the eruption and its eventual release into the stellar wind. Escaping CME events, weakly suppressed by the large-scale field, induce a flare-like signature in the emission from coronal material at different temperatures due to compression and associated heating. …”
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    Coronal response to magnetically-suppressed CME events in M-dwarf stars
  16. 456
    por Balibrea-Correa, J., Babiano-Suarez, V., Lerendegui-Marco, J., Domingo-Pardo, C., Ladarescu, I., Tarifeño-Saldivia, A., Alcayne, V., Cano-Ott, D., González-Romero, E., Martínez, T., Mendoza, E., Plaza, J., Sánchez-Caballero, A., Calviño, F., Casanovas, A., Guerrero, C., Heinitz, S., Köster, U., Maugeri, E.A., Dressler, R., Schumann, D., Mönch, I., Cristallo, S., Lederer-Woods, C., Aberle, O., Altieri, S., Amaducci, S., Andrzejewski, J., Bacak, M., Beltrami, C., Bennett, S., Bernardes, A.P., Berthoumieux, E., Boromiza, M., Bosnar, D., Caamaño, M., Calviani, M., Cerutti, F., Cescutti, G., Chasapoglou, S., Chiaveri, E., Colombetti, P., Colonna, N., Camprini, P. Console, Cortés, G., Cortés-Giraldo, M.A., Cosentino, L., Dellmann, S., Di Castro, M., Di Maria, S., Diakaki, M., Dietz, M., Dupont, E., Durán, I., Eleme, Z., Fargier, S., Fernández, B., Fernández-Domínguez, B., Finocchiaro, P., Fiore, S., Furman, V., García-Infantes, F., ˛ega, A. Gawlik-Rami, Gawlik-Ramięga, A., Gervino, G., Gilardoni, S., Gunsing, F., Gustavino, C., Heyse, J., Hillman, W., Jenkins, D.G., Jericha, E., Junghans, A., Kadi, Y., Kaperoni, K., Kaur, G., Kimura, A., Knapová, I., Kokkoris, M., Kopatch, Y., Krticka, M., Kyritsis, N., Lerner, G., Manna, A., Masi, A., Massimi, C., Mastinu, P., Mastromarco, M., Mazzone, A., Mengoni, A., Michalopoulou, V., Milazzo, P.M., Mucciola, R., Murtas, F., Musacchio-Gonzalez, E., Musumarra, A., Negret, A., de Rada, A. Pérez, Pérez-Maroto, P., Patronis, N., Pavón-Rodríguez, J.A., Pellegriti, M.G., Perkowski, J., Petrone, C., Pirovano, E., Pomp, S., Porras, I., Praena, J., Quesada, J.M., Reifarth, R., Rochman, D., Romanets, Y., Rubbia, C., Sabaté-Gilarte, M., Schillebeeckx, P., Sekhar, A., Smith, A.G., Sosnin, N.V., Stamati, M.E., Sturniolo, A., Tagliente, G., Tarrío, D., Torres-Sánchez, P., Urlass, S., Vagena, E., Valenta, S., Variale, V., Vaz, P., Vecchio, G., Vescovi, D., Vlachoudis, V., Vlastou, R., Wallner, T., Woods, P.J., Wright, T., Zarrella, R., Žugec, P.
    Publicado 2023
    “…One of the crucial ingredients for the improvement of stellar models is the accurate knowledge of neutron capture cross-sections for the different isotopes involved in the $s$-,$r$- and $i$- processes. …”
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    First measurement of the $^{94}$Nb($n$,$\gamma$) cross section at the CERN n_TOF facility
  17. 457
    “…Two kinds of NIVs, Curative Flexo ST30 and Resmed Stellar™ 150, were selected, with S/T mode, respiratory rate of 10 bpm and inspiration time of 1.0 s. …”
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    Factors affecting abnormal triggering with non‐invasive ventilators: A before‐and‐after study
  18. 458
    por Necib, Lina
    Publicado 2022
    “…I first discuss the implications of the different stellar components on direct detection experiments. …”
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    Tracing Dark Matter with Stars around the Milky Way
  19. 459
    por Babiano-Suarez, V, Aberle, O, Alcayne, V, Amaducci, S, Andrzejewski, J, Audouin, L, Bacak, M, Balibrea-Correa, J, Barbagallo, M, Bennett, S, Berthoumieux, E, Bosnar, D, Brown, A S, Busso, M, Caamaño, M, Caballero, L, Calviani, M, Calviño, F, Cano-Ott, D, Casanovas, A, Cerutti, F, Chiaveri, E, Colonna, N, Cortés, G P, Cortés-Giraldo, M A, Cosentino, L, Cristallo, S, Damone, L A, Davies, P J, Diakaki, M, Dietz, M, Domingo-Pardo, C, Dressler, R, Ducasse, Q, Dupont, E, Durán, I, Eleme, Z, Fernández-Domíngez, B, Ferrari, A, Ferro-Gonçalves, I, Finocchiaro, P, Furman, V, Garg, R, Gawlik, A, Gilardoni, S, Göbel, K, González-Romero, E, Guerrero, C, Gunsing, F, Heinitz, S, Heyse, J, Jenkins, D G, Jericha, E, Jiri, U, Junghans, A, Kadi, Y, Käppeler, F, Kimura, A, Knapová, I, Kokkoris, M, Kopatch, Y, Krticka, M, Kurtulgil, D, Ladarescu, I, Lederer-Woods, C, Lerendegui-Marco, J, Lonsdale, S J, Macina, D, Manna, A, Martínez, T, Masi, A, Massimi, C, Mastinu, P F, Mastromarco, M, Maugeri, E, Mazzone, A, Mendoza, E, Mengoni, A, Michalopoulou, V, Milazzo, P M, Millán-Callado, M A, Mingrone, F, Moreno-Soto, J, Musumarra, A, Negret, A, Ogállar, F, Oprea, A, Patronis, N, Pavlik, A, Perkowski, J, Petrone, C, Piersanti, L, Pirovano, E, Porras, I, Praena, J, Quesada, J M, Ramos Doval, D, Reifarth, R, Rochman, D, Rubbia, C, Sabaté-Gilarte, M, Saxena, A, Schillebeeckx, P, Schumann, D, Sekhar, A, Smith, A G, Sosnin, N, Sprung, P, Stamatopoulos, A, Tagliente, G, Tain, J L, Tarifeño-Saldivia, A E, Tassan-Got, L, Thomas, B, Torres-Sánchez, P, Tsinganis, A, Urlass, S, Valenta, S, Vannini, G, Variale, V, Vaz, P, Ventura, A, Vescovi, D, Vlachoudis, V, Vlastou, R, Wallner, A, Woods, P J, Wright, T J, Žugec, P
    Publicado 2020
    “…Particularly relevant are branching nuclei along the s-process path, which are sensitive to the physical conditions of the stellar environment. One such example is the branching at $^{79} \mathrm{Se}$ (3.27 × $10^{5}$ y), which shows a thermally dependent β-decay rate. …”
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    $^{80}$Se(n,$\gamma$) cross-section measurement at CERN n_TOF
  20. 460
    “…The relaxometric and magnetothermal features of IO@STMS or IO@WLMS core shell NPs having respectively stellar or worm-like morphologies are compared and discussed to understand the role of the pore structure for MRI and magnetic hyperthermia applications.…”
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    Orienting the Pore Morphology of Core-Shell Magnetic Mesoporous Silica with the Sol-Gel Temperature. Influence on MRI and Magnetic Hyperthermia Properties
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