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681por Kogure, Tomokazu“…Astrophysics essentially arose in three separate fields: astronomical spectroscopy, stellar structure, and survey of celestial objects. …”
Publicado 2021
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682“…About 1/3 of the 352 pages contain the following Reviews: The Violent Interstellar Medium in Dwarf Galaxies: Atomic Gas (Elias Brinks and Fabian Walter), Hot Gas in the Large Magellanic Cloud (You-Hua Chu), Astrophysics of Dwarf Galaxies: Structures and Stellar Populations (John S. Gallagher), Star-forming regions and ionized gas in irregular galaxies (Deidre A. …”
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683por CERN. Geneva“…Solar neutrino experiments can therefore test both the standard theory of stellar evolution and neutrino properties over a long distance, much larger than the diameter of Earth. (0 refs).…”
Publicado 2000
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684por Barth, K, Passardi, Giorgio, Pezzetti, M, Pirotte, O, Riege, H, Vullierme, B, Walckiers, L, Zioutas, Konstantin“…If existing, axions should be copiously produced in stellar interiors and there are theoretical expectations for a low-energy axion emission spectrum peaked around a mean energy of ~ 4.4 keV. …”
Publicado 2002
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685“…Nature has sprinkled black holes of various sizes throughout the universe, from stellar mass black holes in X-ray sources to supermassive black holes of billions of solar masses in quasars. …”
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686por Amaducci, Simone, Colonna, Nicola, Cosentino, Luigi, Cristallo, Sergio, Finocchiaro, Paolo, Krtička, Milan, Massimi, Cristian, Mastromarco, Mario, Mazzone, Annamaria, Mengoni, Alberto, Valenta, Stanislav, Aberle, Oliver, Alcayne, Victor, Andrzejewski, Józef, Audouin, Laurent, Babiano-Suarez, Victor, Bacak, Michael, Barbagallo, Massimo, Bennett, Samuel, Berthoumieux, Eric, Billowes, Jon, Bosnar, Damir, Brown, Adam, Busso, Maurizio, Caamaño, Manuel, Caballero-Ontanaya, Luis, Calviño, Francisco, Calviani, Marco, Cano-Ott, Daniel, Casanovas, Adria, Cerutti, Francesco, Chiaveri, Enrico, Cortés, Guillem, Cortés-Giraldo, Miguel, Damone, Lucia-Anna, Davies, Paul-John, Diakaki, Maria, Dietz, Mirco, Domingo-Pardo, Cesar, Dressler, Rugard, Ducasse, Quentin, Dupont, Emmeric, Durán, Ignacio, Eleme, Zinovia, Fernández-Domínguez, Beatriz, Ferrari, Alfredo, Furman, Valter, Göbel, Kathrin, Garg, Ruchi, Gawlik, Aleksandra, Gilardoni, Simone, Gonçalves, Isabel, González-Romero, Enrique, Guerrero, Carlos, Gunsing, Frank, Harada, Hideo, Heinitz, Stephan, Heyse, Jan, Jenkins, David, Junghans, Arnd, Käppeler, Franz, Kadi, Yacine, Kimura, Atsushi, Knapova, Ingrid, Kokkoris, Michael, Kopatch, Yuri, Kurtulgil, Deniz, Ladarescu, Ion, Lederer-Woods, Claudia, Leeb, Helmut, Lerendegui-Marco, Jorge, Lonsdale, Sarah-Jane, Macina, Daniela, Manna, Alice, Martínez, Trinitario, Masi, Alessandro, Mastinu, Pierfrancesco, Maugeri, Emilio-Andrea, Mendoza, Emilio, Michalopoulou, Veatriki, Milazzo, Paolo, Mingrone, Federica, Moreno-Soto, Javier, Musumarra, Agatino, Negret, Alexandru, Ogállar, Francisco, Oprea, Andreea, Patronis, Nikolas, Pavlik, Andreas, Perkowski, Jarosław, Piersanti, Luciano, Petrone, Cristina, Pirovano, Elisa, Porras, Ignacio, Praena, Javier, Quesada, José-Manuel, Ramos-Doval, Diego, Rauscher, Thomas, Reifarth, René, Rochman, Dimitri, Rubbia, Carlo, Sabaté-Gilarte, Marta, Saxena, Alok, Schillebeeckx, Peter, Schumann, Dorothea, Sekhar, Adhitya, Smith, Gavin, Sosnin, Nikolay, Sprung, Peter, Stamatopoulos, Athanasios, Tagliente, Giuseppe, Tain, José, Tarifeño-Saldivia, Ariel, Tassan-Got, Laurent, Thomas, Benedikt, Torres-Sánchez, Pablo, Tsinganis, Andrea, Ulrich, Jiri, Urlass, Sebastian, Vannini, Gianni, Variale, Vincenzo, Vaz, Pedro, Ventura, Alberto, Vescovi, Diego, Vlachoudis, Vasilis, Vlastou, Rosa, Wallner, Anton, Woods, PhilipJohn, Wright, Tobias, Žugec, Petar“…The measurement was motivated by the significant difference between the cerium abundance measured in globular clusters and the value predicted by theoretical stellar models. This discrepancy can be ascribed to an overestimation of the $^{140}$Ce capture cross-section due to a lack of accurate nuclear data. …”
Publicado 2021
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687por Lerendegui-Marco, J., Alcayne, V., Babiano-Suarez, V., Bacak, M., Balibrea-Correa, J., Casanovas, A., Domingo-Pardo, C., de la Fuente, G., Gameiro, B., García-Infantes, F., Ladarescu, I., Musacchio-Gonzalez, E., Pavón-Rodríguez, J.A., Tarifeño-Saldivia, A.“…One of the best suited methods to measure radiative neutron capture (n,$\gamma$) cross sections over the full stellar range of interest for all the applications is the time-of-flight (TOF) technique. …”
Publicado 2023
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688por Gratton, Raffaele, Mesa, Dino, Bonavita, Mariangela, Zurlo, Alice, Marino, Sebastian, Kervella, Pierre, Desidera, Silvano, D’Orazi, Valentina, Rigliaco, Elisabetta“…However, they may be much more common in one of the closest associations in the solar neighbourhood. Young moving stellar groups are the best targets for direct imaging of exoplanets and four massive Jupiter-like planets have been already discovered in the nearby young β Pic Moving Group (BPMG) via high-contrast imaging, and four others were suggested via high precision astrometry by the European Space Agency’s Gaia satellite. …”
Publicado 2023
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689“…Strength-duration data for the giant fiber of the great stellar nerve of the squid (Loligo pealii) can be approximately described by several mathematical formulations. 2. …”
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690“…This report is the first observation of high-brightness random Q-switched laser emission and is expected to stimulate new areas of scientific research and applications, including encryption, remote three-dimensional random imaging and the simulation of stellar lasing.…”
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691por Chen, Yan-Mei, Shi, Yong, Tremonti, Christy A., Bershady, Matt, Merrifield, Michael, Emsellem, Eric, Jin, Yi-Fei, Huang, Song, Fu, Hai, Wake, David A., Bundy, Kevin, Stark, David, Lin, Lihwai, Argudo-Fernandez, Maria, Bergmann, Thaisa Storchi, Bizyaev, Dmitry, Brownstein, Joel, Bureau, Martin, Chisholm, John, Drory, Niv, Guo, Qi, Hao, Lei, Hu, Jian, Li, Cheng, Li, Ran, Lopes, Alexandre Roman, Pan, Kai-Ke, Riffel, Rogemar A., Thomas, Daniel, Wang, Lan, Westfall, Kyle, Yan, Ren-Bin“…The central regions of blue counter-rotators show younger stellar populations and more intense, ongoing star formation than their outer parts, indicating ongoing growth of the central regions. …”
Publicado 2016
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692“…The knowledge of the metallization of warm dense helium has important implications for understanding the thermal histories, stellar structure and magnetic field environment of giant planets. …”
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693por Bailly-Grandvaux, M., Santos, J. J., Bellei, C., Forestier-Colleoni, P., Fujioka, S., Giuffrida, L., Honrubia, J. J., Batani, D., Bouillaud, R., Chevrot, M., Cross, J. E., Crowston, R., Dorard, S., Dubois, J.-L., Ehret, M., Gregori, G., Hulin, S., Kojima, S., Loyez, E., Marquès, J.-R., Morace, A., Nicolaï, Ph., Roth, M., Sakata, S., Schaumann, G., Serres, F., Servel, J., Tikhonchuk, V. T., Woolsey, N., Zhang, Z.“…Such an improvement of energy-density flux through dense matter paves the ground for advances in laser-driven intense sources of energetic particles and radiation, driving matter to extreme temperatures, reaching states relevant for planetary or stellar science as yet inaccessible at the laboratory scale and achieving high-gain laser-driven thermonuclear fusion.…”
Publicado 2018
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694por Middleton, Hannah, Chen, Siyuan, Del Pozzo, Walter, Sesana, Alberto, Vecchio, Alberto“…The stringent upper limit from the Parkes Pulsar Timing Array has been interpreted as excluding (>90% confidence) the current paradigm of binary assembly through galaxy mergers and hardening via stellar interaction, suggesting evolution is accelerated or stalled. …”
Publicado 2018
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695“…Here, we present an observation of how a stellar-sized CME bubble evolves continuously from plasmoids, mini flux ropes that are barely resolved, within half an hour. …”
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696por Mabey, P., Albertazzi, B., Falize, E., Michel, Th., Rigon, G., Van Box Som, L., Pelka, A., Brack, F.-E., Kroll, F., Filippov, E., Gregori, G., Kuramitsu, Y., Lamb, D. Q., Li, C., Ozaki, N., Pikuz, S., Sakawa, Y., Tzeferacos, P., Koenig, M.“…A stationary shock is formed, several hundred kilometres above the stellar surface; a distance far too small to be resolved with today’s telescopes. …”
Publicado 2019
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697por Farahi, Arya, Mulroy, Sarah L., Evrard, August E., Smith, Graham P., Finoguenov, Alexis, Bourdin, Hervé, Carlstrom, John E., Haines, Chris P., Marrone, Daniel P., Martino, Rossella, Mazzotta, Pasquale, O’Donnell, Christine, Okabe, Nobuhiro“…The largest clusters of galaxies in the Universe contain vast amounts of dark matter, plus baryonic matter in two principal phases, a majority hot gas component and a minority cold stellar phase comprising stars, compact objects, and low-temperature gas. …”
Publicado 2019
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698por Damasso, Mario, Del Sordo, Fabio, Anglada-Escudé, Guillem, Giacobbe, Paolo, Sozzetti, Alessandro, Morbidelli, Alessandro, Pojmanski, Grzegorz, Barbato, Domenico, Butler, R. Paul, Jones, Hugh R. A., Hambsch, Franz-Josef, Jenkins, James S., López-González, María José, Morales, Nicolás, Peña Rojas, Pablo A., Rodríguez-López, Cristina, Rodríguez, Eloy, Amado, Pedro J., Anglada, Guillem, Feng, Fabo, Gómez, Jose F.“…The analysis of photometric data and spectro-scopic activity diagnostics does not explain the signal in terms of a stellar activity cycle, but follow-up is required in the coming years for confirming its planetary origin. …”
Publicado 2020
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699por Boutle, Ian A., Joshi, Manoj, Lambert, F. Hugo, Mayne, Nathan J., Lyster, Duncan, Manners, James, Ridgway, Robert, Kohary, Krisztian“…Yet habitability depends not only on the stellar irradiance, but equally on constituent parts of the planetary atmosphere. …”
Publicado 2020
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700“…Optical emission lines are used to categorize galaxies into three groups according to their dominant central radiation source: active galactic nuclei, star formation, or low-ionization (nuclear) emission regions [LI(N)ERs] that may trace ionizing radiation from older stellar populations. Using the Wisconsin H-Alpha Mapper, we detect optical line emission in low-extinction windows within eight degrees of Galactic Center. …”
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