Results 111 to 120 of about 130,560 (227)
Quark nova imprint in the extreme supernova explosion SN 2006gy
The extremely luminous supernova 2006gy (SN 2006gy) is among the most
energetic ever observed. The peak brightness was 100 times that of a typical
supernova and it spent an unheard of 250 days at magnitude -19 or brighter.Agnoletto, Bodmer, Chatzopoulos, D. A. Leahy, Drake, Dwarkadas, Gal-Yam, Gezari, Heger, Itoh, Jaikumar, Keränen, Leahy, M. Kostka, Mihalas, Miller, Miller, N. Koning, Niebergal, Ofek, Ouyed, Ouyed, Ouyed, Ouyed, Quimby, R. Ouyed, Rest, Smith, Smith, Staff, Steffen, Umeda, Vogt, W. Steffen, Witten, Woosley, Yungelson +36 morecore +2 more sourcesThe Search for Supernova-produced Radionuclides in Terrestrial Deep-sea
Archives
An enhanced concentration of 60Fe was found in a deep ocean's crust in 2004
in a layer corresponding to an age of ~2 Myr. The confirmation of this signal
in terrestrial archives as supernova-induced and detection of other
supernova-produced radionuclides A. Wallner, Aggarwal, Allison, Auer, Avillez, Berghöfer, Bourlès, Chmeleff, Cook, D. Breitschwerdt, Diehl, Fitoussi, Fitoussi, Fuchs, G. Korschinek, G. Rugel, Hofmann, Holden, Honda, Imamura, J. Feige, Knie, Knie, Korschinek, Korschinek, L. K. Fifield, Lachner, Merchel, Middleton, Nishiizumi, Paul, Paul, Rugel, S. Merchel, S. R. Winkler, Samworth, Thomas, Wallner +37 morecore +2 more sourcesShocks and Particle Acceleration in Supernova Remnants: Observational
Features
The last ten years a number of observational advances have substantially
increased our knowledge of shock phenomena in supernova remnants. This progress
has mainly been made possible by the recent improvements in X-ray and Gamma-ray
instrumentation.Aharonian, Allen, Allen, Atoyan, Bamba, Bell, Bell, Bell, Berezhko, Biermann, Blandford, Bleeker, Borkowski, Butt, Bykov, Bykov, Cowsik, Decourchelle, Delaney, Dyer, Eichler, Enomoto, Favata, Ghavamian, Ghavamian, Gotthelf, Hamilton, Hughes, Hunter, Itoh, Jacco Vink, Jones, Koyama, Koyama, Lagage, Laming, Laming, Laming, Longair, Malkov, McKee, Muraishi, Reed, Reimer, Reynolds, Reynolds, Reynolds, Rho, Schmitz, Schmitz, Slane, Slane, Smith, Stephenson, Tanimori, Torres, van der Laan, Vink, Vink, Vink, Vink, Vink, Vink, Zeldovich +63 morecore +2 more sourcesDetection of a close supernova gravitational wave burst in a network of
interferometers, neutrino and optical detectors
Trying to detect the gravitational wave (GW) signal emitted by a type II
supernova is a main challenge for the GW community. Indeed, the corresponding
waveform is not accurately modeled as the supernova physics is very complex; in
addition, all the ...Anderson, Anderson, Arnaud, Arnaud, Arnaud, Arnaud, Arnaud, Arnaud, Baryshev, Beacom, Beacom, Boger, Bonazzola, Bonnel, Burrows, Cappellaro, Creighton, Cuoco, Cuoco, Dimmelmeier, Dimmelmeier, Edward K. Porter, Fabien Cavalier, Ferrari, Finn, Fukuda, Helstrom, Lobashev, Marie-Anne Bizouard, Matteo Barsuglia, Michel Davier, Mohanty, Mönchneyer, Nakano, Nazin, Nicolas Arnaud, Owen, Pai, Panagia, Patrice Hello, Pradier, Press, Searle, Searle, Spergel, Stark, Stephane Kreckelbergh, Sylvestre, Sylvestre, Teukolsky, Thorne, Tully, Viceré, Violette Brisson, Wainstein, Weinheimer, Yamada, Zwerger +57 morecore +2 more sourcesReducing Zero-point Systematics in Dark Energy Supernova Experiments [PDF]
We study the effect of filter zero-point uncertainties on future supernova
dark energy missions. Fitting for calibration parameters using simultaneous
analysis of all Type Ia supernova standard candles achieves a significant
improvement over more ...A. Bonissent, A. Stebbins, A.G. Kim, Aldering, Amanullah, Astier, Branch, C. Stoughton, Cardelli, Copin, D. Gerdes, D. Tucker, Dawson, de Putter, E.V. Linder, G. Bernstein, G. Kushner, H. Shukla, Hicken, Hsiao, J. Christiansen, Kim, Kim, Kowalski, L. Faccioli, L. Gladney, Linder, Linder, Linder, M. Brown, N. Connolly, N. Mostek, Nordin, Perlmutter, Perlmutter, R. Miquel, Riess, S. Deustua, S. McKee, Samsing, W. Carithers, Wood-Vasey +41 morecore +1 more sourceRadioactive Probes of the Supernova-Contaminated Solar Nebula: Evidence
that the Sun was Born in a Cluster [PDF]
We construct a simple model for radioisotopic enrichment of the protosolar
nebula by injection from a nearby supernova, based on the inverse square law
for ejecta dispersion.Brian D. Fields, Cosarinsky M., Hauri E. H., John J. Tobin, Kleine T., Kleine T., Leslie W. Looney, Meyer B. S., Meyer B. S., Nyquist L. E., Yorke H. W., Young E. D. +11 morecore +1 more sourcePerformance of SK-Gd’s Upgraded Real-time Supernova Monitoring System
The Astrophysical JournalAmong multimessenger observations of the next Galactic core-collapse supernova, Super-Kamiokande (SK) plays a critical role in detecting the emitted supernova neutrinos, determining the direction to the supernova (SN), and notifying the astronomical ...Y. Kashiwagi, K. Abe, C. Bronner, Y. Hayato, K. Hiraide, K. Hosokawa, K. Ieki, M. Ikeda, J. Kameda, Y. Kanemura, R. Kaneshima, Y. Kataoka, S. Miki, S. Mine, M. Miura, S. Moriyama, Y. Nakano, M. Nakahata, S. Nakayama, Y. Noguchi, K. Sato, H. Sekiya, H. Shiba, K. Shimizu, M. Shiozawa, Y. Sonoda, Y. Suzuki, A. Takeda, Y. Takemoto, H. Tanaka, T. Yano, S. Han, T. Kajita, K. Okumura, T. Tashiro, T. Tomiya, X. Wang, S. Yoshida, P. Fernandez, L. Labarga, N. Ospina, B. Zaldivar, B. W. Pointon, E. Kearns, J. L. Raaf, L. Wan, T. Wester, J. Bian, N. J. Griskevich, S. Locke, M. B. Smy, H. W. Sobel, V. Takhistov, A. Yankelevich, J. Hill, M. C. Jang, S. H. Lee, D. H. Moon, R. G. Park, B. Bodur, K. Scholberg, C. W. Walter, A. Beauchêne, O. Drapier, A. Giampaolo, Th. A. Mueller, A. D. Santos, P. Paganini, B. Quilain, R. Rogly, T. Nakamura, J. S. Jang, L. N. Machado, J. G. Learned, K. Choi, N. Iovine, S. Cao, L. H. V. Anthony, D. Martin, N. W. Prouse, M. Scott, A. A. Sztuc, Y. Uchida, V. Berardi, M. G. Catanesi, E. Radicioni, N. F. Calabria, A. Langella, G. De Rosa, G. Collazuol, F. Iacob, M. Mattiazzi, L. Ludovici, M. Gonin, L. Périssé, G. Pronost, C. Fujisawa, Y. Maekawa, Y. Nishimura, R. Okazaki, R. Akutsu, M. Friend, T. Hasegawa, T. Ishida, T. Kobayashi, M. Jakkapu, T. Matsubara, T. Nakadaira, K. Nakamura, Y. Oyama, K. Sakashita, T. Sekiguchi, T. Tsukamoto, N. Bhuiyan, G. T. Burton, F. Di Lodovico, J. Gao, A. Goldsack, T. Katori, J. Migenda, R. M. Ramsden, Z. Xie, S. Zsoldos, A. T. Suzuki, Y. Takagi, Y. Takeuchi, H. Zhong, J. Feng, L. Feng, J. R. Hu, Z. Hu, M. Kawaue, T. Kikawa, M. Mori, T. Nakaya, R. A. Wendell, K. Yasutome, S. J. Jenkins, N. McCauley, P. Mehta, A. Tarrant, Y. Fukuda, Y. Itow, H. Menjo, K. Ninomiya, Y. Yoshioka, J. Lagoda, S. M. Lakshmi, M. Mandal, P. Mijakowski, Y. S. Prabhu, J. Zalipska, M. Jia, J. Jiang, C. K. Jung, W. Shi, M. J. Wilking, C. Yanagisawa, M. Harada, Y. Hino, H. Ishino, Y. Koshio, F. Nakanishi, S. Sakai, T. Tada, T. Tano, T. Ishizuka, G. Barr, D. Barrow, L. Cook, S. Samani, D. Wark, A. Holin, F. Nova, S. Jung, B. S. Yang, J. Y. Yang, J. Yoo, J. E. P. Fannon, L. Kneale, M. Malek, J. M. McElwee, M. D. Thiesse, L. F. Thompson, S. T. Wilson, H. Okazawa, S. B. Kim, E. Kwon, J. W. Seo, I. Yu, A. K. Ichikawa, K. D. Nakamura, S. Tairafune, K. Nishijima, A. Eguchi, K. Nakagiri, Y. Nakajima, S. Shima, N. Taniuchi, E. Watanabe, M. Yokoyama, P. de Perio, S. Fujita, C. Jesús-Valls, K. Martens, K. M. Tsui, M. R. Vagins, J. Xia, M. Kuze, S. Izumiyama, R. Matsumoto, M. Ishitsuka, H. Ito, Y. Ommura, N. Shigeta, M. Shinoki, K. Yamauchi, T. Yoshida, R. Gaur, V. Gousy-Leblanc, M. Hartz, A. Konaka, X. Li, S. Chen, B. D. Xu, B. Zhang, M. Posiadala-Zezula, S. B. Boyd, R. Edwards, D. Hadley, M. Nicholson, M. O’Flaherty, B. Richards, A. Ali, B. Jamieson, S. Amanai, Ll. Marti, A. Minamino, S. Suzuki, The Super-Kamiokande Collaboration +239 moredoaj +1 more sourceSupernova remnant S147 and its associated neutron star(s)
The supernova remnant S147 harbors the pulsar PSR J0538+2817 whose
characteristic age is more than an order of magnitude greater than the
kinematic age of the system (inferred from the angular offset of the pulsar
from the geometric center of the ...Anderson, Arnal, Bethe, Blondin, Bock, Cioffi, Colpi, Cordes, Drew, Fesen, Fürst, Gaensler, Gondhalekar, Gott, Gvaramadze, Gvaramadze, Gvaramadze, Hobbs, Iben, Illarionov, Kirshner, Kramer, Kundu, Lewandowski, Lozinskaya, Manchester, McGowan, Migliazzo, Milne, Morris, Ng, Phillips, Phillips, Reich, Romani, Sallmen, Sofue, Souvageot, Spruit, Sun, Tauris, Tenorio-Tagle, V. V. Gvaramadze, van Buren, van den Bergh, Vanbeveren, Vlemmings, Wex, Yakovlev +48 morecore +2 more sources
