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741por Dillmann, Iris, Kester, Oliver, Baartman, Richard, Chen, Alan, Junginger, Tobias, Herwig, Falk, Kaltchev, Dobrin, Lennarz, Annika, Planche, Thomas, Ruiz, Chris, Vassh, Nicole“…For decades, the precise measurement of direct neutron capture cross sections in the “stellar” energy range (eV up to a few MeV) was limited to stable and longer-lived nuclei that could be provided as physical samples and then irradiated with neutrons. …”
Publicado 2023
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742“…Properties of nuclei in hot stellar environments such as supernovae or neutron star mergers are largely unexplored. …”
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743por Krestianinov, Evgenii, Amelin, Yuri, Yin, Qing-Zhu, Cary, Paige, Huyskens, Magdalena H., Miller, Audrey, Dey, Supratim, Hibiya, Yuki, Tang, Haolan, Young, Edward D., Pack, Andreas, Di Rocco, Tommaso“…Here we demonstrate that the current data clearly indicate spatial heterogeneity of (26)Al by a factor of 3-4 in the precursor molecular cloud or the protoplanetary disk of the Solar System, likely associated with the late infall of stellar materials with freshly synthesized radionuclides.…”
Publicado 2023
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744por Fougères, Chloé, de Oliveira Santos, François, José, Jordi, Michelagnoli, Caterina, Clément, Emmanuel, Kim, Yung Hee, Lemasson, Antoine, Guimarães, Valdir, Barrientos, Diego, Bemmerer, Daniel, Benzoni, Giovanna, Boston, Andrew J., Böttger, Roman, Boulay, Florent, Bracco, Angela, Čeliković, Igor, Cederwall, Bo, Ciemala, Michał, Delafosse, Clément, Domingo-Pardo, César, Dudouet, Jérémie, Eberth, Jürgen, Fülöp, Zsolt, González, Vicente, Gottardo, Andrea, Goupil, Johan, Hess, Herbert, Jungclaus, Andrea, Kaşkaş, Ayşe, Korichi, Amel, Lenzi, Silvia M., Leoni, Silvia, Li, Hongjie, Ljungvall, Joa, Lopez-Martens, Araceli, Menegazzo, Roberto, Mengoni, Daniele, Million, Benedicte, Mrázek, Jaromír, Napoli, Daniel R., Navin, Alahari, Nyberg, Johan, Podolyák, Zsolt, Pullia, Alberto, Quintana, Begoña, Ralet, Damien, Redon, Nadine, Reiter, Peter, Rezynkina, Kseniia, Saillant, Frédéric, Salsac, Marie-Delphine, Sánchez-Benítez, Angel M., Sanchis, Enrique, Şenyiğit, Menekşe, Siciliano, Marco, Smirnova, Nadezda A., Sohler, Dorottya, Stanoiu, Mihai, Theisen, Christophe, Valiente-Dobón, Jose J., Ujić, Predrag, Zielińska, Magdalena“…Classical novae are thermonuclear explosions in stellar binary systems, and important sources of (26)Al and (22)Na. …”
Publicado 2023
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745por Goobar, Ariel, Johansson, Joel, Schulze, Steve, Arendse, Nikki, Carracedo, Ana Sagués, Dhawan, Suhail, Mörtsell, Edvard, Fremling, Christoffer, Yan, Lin, Perley, Daniel, Sollerman, Jesper, Joseph, Rémy, Hinds, K-Ryan, Meynardie, William, Andreoni, Igor, Bellm, Eric, Bloom, Josh, Collett, Thomas E., Drake, Andrew, Graham, Matthew, Kasliwal, Mansi, Kulkarni, Shri R., Lemon, Cameron, Miller, Adam A., Neill, James D., Nordin, Jakob, Pierel, Justin, Richard, Johan, Riddle, Reed, Rigault, Mickael, Rusholme, Ben, Sharma, Yashvi, Stein, Robert, Stewart, Gabrielle, Townsend, Alice, Vinko, Jozsef, Wheeler, J. Craig, Wold, Avery“…It involves a combination of two very rare phenomena: catching the transient signal of a stellar explosion in a distant galaxy and observing it through a nearly perfectly aligned foreground galaxy that deflects light towards the observer. …”
Publicado 2023
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746por Anders, Evan H., Lecoanet, Daniel, Cantiello, Matteo, Burns, Keaton J., Hyatt, Benjamin A., Kaufman, Emma, Townsend, Richard H. D., Brown, Benjamin P., Vasil, Geoffrey M., Oishi, Jeffrey S., Jermyn, Adam S.“…We present three-dimensional simulations of massive star convection extending from the star’s centre to near its surface, with realistic stellar luminosities. Using these simulations, we predict the photometric variability due to convectively driven gravity waves at the surfaces of massive stars, and find that gravity waves produce photometric variability of a lower amplitude and lower characteristic frequency than the observed red noise. …”
Publicado 2023
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747por Li, Xuemei, Huang, Wengang, Krajnc, Andraž, Yang, Yuwei, Shukla, Atul, Lee, Jaeho, Ghasemi, Mehri, Martens, Isaac, Chan, Bun, Appadoo, Dominique, Chen, Peng, Wen, Xiaoming, Steele, Julian A., Hackbarth, Haira G., Sun, Qiang, Mali, Gregor, Lin, Rijia, Bedford, Nicholas M., Chen, Vicki, Cheetham, Anthony K., Tizei, Luiz H. G., Collins, Sean M., Wang, Lianzhou, Hou, Jingwei“…The stellar optoelectronic properties of metal halide perovskites provide enormous promise for next-generation optical devices with excellent conversion efficiencies and lower manufacturing costs. …”
Publicado 2023
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748An Autonomous Star Identification Algorithm Based on One-Dimensional Vector Pattern for Star Sensors“…The one-dimensional vector pattern of the same observed star remains unchanged when the stellar image rotates, so the problem of star identification is simplified as the comparison of the two feature vectors. …”
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749por Goldt, Sebastian, Advani, Madhu S, Saxe, Andrew M, Krzakala, Florent, Zdeborová, Lenka“…Deep neural networks achieve stellar generalisation even when they have enough parameters to easily fit all their training data. …”
Publicado 2020
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750“…Moreover, we studied the hydrostatic equilibrium of the stellar system by using a modified TOV equation and the dynamical stability through the critical value of the radial adiabatic index. …”
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751por Samanta, Tanmoy, Tian, Hui, Chen, Bin, Reeves, Katharine K., Cheung, Mark C.M., Vourlidas, Angelos, Banerjee, Dipankar“…Several of these interactions generate clear signatures of quasi-periodic enhancement in the full-Sun-integrated soft X-ray emission, providing an alternative interpretation for quasi-periodic pulsations that are commonly observed during solar and stellar flares.…”
Publicado 2021
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752por Gatchell, Michael, Ameixa, João, Ji, MingChao, Stockett, Mark H., Simonsson, Ansgar, Denifl, Stephan, Cederquist, Henrik, Schmidt, Henning T., Zettergren, Henning“…Here we study the survival of reactive fragments of the polycyclic aromatic hydrocarbon (PAH) coronene, where individual C atoms have been knocked out of the molecules in hard collisions with He atoms at stellar wind and supernova shockwave velocities. Ionic fragments are stored in the DESIREE cryogenic ion-beam storage ring where we investigate their decay for up to one second. …”
Publicado 2021
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753“…The representation of magnetic field as a sum of a toroidal field and a poloidal field has not rarely been used in astrophysics, particularly in relation to stellar and planetary magnetism. In this representation, each toroidal field line lies entirely in a surface, which is named a toroidal field surface. …”
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754por Yan, Hongliang, Li, Haining, Wang, Song, Zong, Weikai, Yuan, Haibo, Xiang, Maosheng, Huang, Yang, Xie, Jiwei, Dong, Subo, Yuan, Hailong, Bi, Shaolan, Chu, Yaoquan, Cui, Xiangqun, Deng, Licai, Fu, Jianning, Han, Zhanwen, Hou, Jinliang, Li, Guoping, Liu, Chao, Liu, Jifeng, Liu, Xiaowei, Luo, Ali, Shi, Jianrong, Wu, Xuebing, Zhang, Haotong, Zhao, Gang, Zhao, Yongheng“…The LAMOST survey covers various objects in the Universe, from normal stars to peculiar ones, from the Milky Way to other galaxies, and from stellar black holes and their companions to quasars that ignite ancient galaxies. …”
Publicado 2022
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755por Dereli-Bégué, Hüsne, Pe’er, Asaf, Ryde, Felix, Oates, Samantha R., Zhang, Bing, Dainotti, Maria G.“…Furthermore, long GRB progenitors are either not Wolf-Rayet stars, or the wind properties during the final stellar evolution phase are different than at earlier times. …”
Publicado 2022
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756por Coupechoux, J.-F., Arbey, A., Chierici, R., Hansen, H., Margueron, J., Sordini, V.“…In the absence of discriminating power based on the gravitational waveforms, the classification of sources into binary neutron stars, binary black holes and mixed systems can only be unambiguous when assuming the standard model of stellar evolution and using the fact that there exists a mass gap between neutron stars and black holes. …”
Publicado 2021
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757por Darnley, Matt J., Bode, M.F., Kerins, E., Newsam, A.M., An, J., Baillon, P., Calchi Novati, S., Carr, Bernard J., Creze, M., Evans, N.W., Giraud-Heraud, Y., Gould, A., Hewett, Paul C., Jetzer, Ph., Kaplan, J., Paulin-Henriksson, S., Smartt, S.J., Stalin, C.S., Tsapras, Y.“…The CN catalogue constitutes a uniquely well-sampled and objectively-selected data set with which to study the statistical properties of classical novae in M31, such as the global nova rate, the reliability of novae as standard-candle distance indicators and the dependence of the nova population on stellar environment. The findings of this statistical study will be reported in a follow-up paper.…”
Publicado 2004
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758“…High resolution here means that lines in cool stellar atmospheres and HII-regions can be resolved. …”
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759por Kyrala, G.A“…The conference brought together different scientists interested in this emerging new filed, with topics covering: - Hydrodynamic instabilities in astrophysics, - Supernovae and supernova remnant evolution, - Aastrophysical shocks, blast waves, and jets, - Stellar opacities, - Radiation and thermal transport, - Dense plasma atomic physics and EOS - X-ray photoionized plasmas, - Ultrastrong magnetic field generation Reprinted from Astrophysics and Space Science, volume 298, Nos. 1-2, 2005…”
Publicado 2005
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760“…These and other new instruments will have a major impact in a wide range of scientific topics including the cosmological epoch of reionization, galactic dynamics and nuclear activity, stellar astronomy, extra-solar planets, gamma-ray bursts, X-ray binaries, and many others. …”
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