Natasha Fairweather, Gerald Stonehill, Jon Ashworth, Brendan Martin, Gerald Isaaman, Mark Mann, Andrew Pierce, Political Correspondent, Paul Heiney, Portia Colwell, Andrew Pierce, Alexandra Frean, Ann Barroll (Chairman), Patricia Davies, Paula Davies, Ivor H. Mills (Professor), Jane MacQuitty, Simon Barnes, Richard Ford, Home Correspondent, Jan Morris, Dr S. Jennings, Paul Hoggart, P . H. S, Emma Haughton, Richard Hobson, John Diamond, W. S. Affleck, Maureen Owen, Judy Goodkin, Gavin Lumsden, Philip Howard, Hilary Finch, G. P., Michael Binyon, Joanna Bale, Rachel Campbell-Johnston, John Trayner, Jack Bannister, Peregrine Cleveland-Peck, Mina Bawden, Nicholas Watt, Chief Ireland Correspondent, Carl Mortished, Richard Evans and Richard Ford, Ginny Dougary, Tony Patrick, Tom Walker, Kevin Eason, Joe Joseph, Louise Godfrey, Carl Evans, Ruth Gledhill, Religion Correspondent, John Clarke, Maurice Owen, Darcey Bussell, Robert Sheehan, Vinny Lee, D. R., Peter Blunt, Feldman, Ruth Gledhill, Debra Craine, Anne Ashworth, Caroline Merrell and Sara McConnell, Gioconda, Ruth Gledhill Religion Correspondent, Dalya Alberge Arts Correspondent, Lord Montagu, Peter Waymark, Richard Ford Home Correspondent, Robin Young, Rodney Milnes, Jenny MacArthur, Timothy Rice, Michael Clark, Eve-Ann Prentice, J. L. Wilson (Author), Helen Dunmore, Jeremy Laurance, Health Correspondent, George Perry, T. P., Frances Bissell, Quentin Letts, Peter Davies, Tessa Souter, P. B., Anna Blundy, David Long and Les Evans, Peter Barnard, Derwent May, Mary Loudon, Lisa Jardine, Brian Crozier, Clare Colvin, Lizanne Rose, Anthony V. Purnell, John K. Roberts, Harvey Elliott, Air Correspondent, Russell Kempson, Anthony Minghella, Linda Galloway, Dick Morris, Oleg Gordievsky, Paul Durman, Stephen Anderton, Annie Henry, Ben MacIntyre and Adrian Lee, Noel Pascoe, Roger Maynard and Michael Evans, Jane Wheatley, Angus Mewse, Paul Myles, L. G., Lin Jenkins, Nathan Yates, Barry Millington, Mitch Jenkins, Arthur Leathley, Political Correspondent, Christina Koning, John Higgins, Dalya Alberge, Arts Correspondent, Adam Jones, John Shaw and Adrian Lee, David Powell Athletics Correspondent, Raymond Keene, Vaughan Freeman, David Robinson, Polly Newton, Emma Wilkins, Leslie Thuillier, John Russell Taylor, Cheryl Taylor, P. W., Lucy Pinney, Alix Ramsay, Paul Wilkinson, James Allcock, P. H. S, Russell Hayes, C. F. Dayer, Richard Evans, Caroline Merrell, Robin Neillands, Bronwen Maddox, Eric Reguly, Richard Owen, David Powell, Athletics Correspondent, Elizabeth McGovern, John Gummer, Martin Alpren, Sarah Cunningham, Erica Wagner, E. J. McFadden, Stephanie Billen, Dalya Alberge, Kathryn Knight and Michael Horsnell, Glen Owen, Adam Fresco, Andrew Pierce and Arthur Leathley, John Allison, Caroline Bonwitt, Christopher Thomas, Anne Ashworth, John Goodbody, Joanna Pitman, Nick Szczepanik, David Churchill, Sara McConnell, Daniel Farson, Christopher Walker, Robert Crampton, Quentin Crewe, Alan Copps, Mel Webb, Nigel Buraham, Gerald Larner, William Oddie, Matthew Parris, Richard Evans Racing Correspondent, Amanda Craig, Alan Franks, Tim Wapshott, Michael Hornsby, Jane Owen, Ben MacIntyre, Russell Jenkins and Glen Owen, Helen Pridham, John Moses, Robert Allen, Ian Brodie, Tony Dawe, Richard Beeston, Eric Lummis, Michael Dynes, Helen Pickles, Graham Searjeant, Jason Cowley, Simon Jenkins, Fraser Nelson, Hattie Ellis, David Sinclair, Heath Brown, Benedict Nightingale, John P. Fox, Stuart Birch, Tom Rhodes, Jonathan Meades, Edward Thomas, Marianne Curphey, Jill Crawshaw, Michael Evans Defence Correspondent, Richard Morrison, Sam Kiley, Caroline Merrell and Sara McConnell, Susan MacDonald, David Maddock, Alasdair Murray, Penny Perrick, David Hands, Rugby Correspondent, Gill Hornby, Christopher Irvine, Frank Yule, Christine Buckley, Industrial Correspondent,
... asks. Portrait by Mitch Jenkins Texas Instruments A shockwave over 5.5 can Damage underground water… The ...
1997 - Gale Group | TDA
Y. Tsubone, Makoto Sawada, Aya Bamba, Satoru Katsuda, Jacco Vink,
ABSTRACT Diffusive shock acceleration by the shockwaves in supernova remnants (SNRs) is widely accepted as the dominant source for Galactic cosmic rays. However, it is unknown what determines the maximum energy ...
Tópico(s): Solar and Space Plasma Dynamics
2017 - IOP Publishing | The Astrophysical Journal
G. E. Anderson, J. C. A. Miller‐Jones, Matthew Middleton, Roberto Soria, Douglas A. Swartz, Ryan Urquhart, N. Hurley‐Walker, P. J. Hancock, R. P. Fender, P. Gandhi, Sera Markoff, T. P. Roberts,
... to rule out other identifications including long-term supernova shockwave interactions with the surrounding medium from a faint supernova or a background active galaxy.
Tópico(s): Galaxies: Formation, Evolution, Phenomena
2019 - Oxford University Press | Monthly Notices of the Royal Astronomical Society
... explanation of gas-phase depletions. We show that supernova shockwaves sweep a significantly larger mass of interstellar gas per unit time than the shockwaves generated by outflows in star-forming regions. We apply our sputtering model to the bombardment levels expected in a supernova shock, and show that net embedding may dominate ...
Tópico(s): Astrophysics and Cosmic Phenomena
2004 - Oxford University Press | Monthly Notices of the Royal Astronomical Society
Michael Gatchell, João Ameixa, MingChao Ji, Mark H. Stockett, A. Simonsson, Stephan Denifl, H. Cederquist, H. T. Schmidt, Henning Zettergren,
... collisions with He atoms at stellar wind and supernova shockwave velocities. Ionic fragments are stored in the DESIREE ...
Tópico(s): Astro and Planetary Science
2021 - Nature Portfolio | Nature Communications
We compute the energy spectra of antideuterons and antihelium in cosmic rays (CRs) in a scenario where hadronic interactions inside supernova remnants (SNRs) can produce a diffusively-shock-accelerated "source component" of secondary antinuclei. The key parameters that specify the SNR environment and the interstellar CR transport are tightly constrained with the new measurements provided by the AMS experiment on the B/C ratio and on the antiproton/proton ratio. The best-fit models obtained from the ...
Tópico(s): Neutrino Physics Research
2017 - IOP Publishing | The Astrophysical Journal Letters
P. Garnavich, B. Tucker, A. Rest, E. Shaya, R. Olling, Daniel Kasen, A. Villar,
... than the models predict possibly due to the supernova shockwave moving into pre-existing wind or mass-loss ...
Tópico(s): Astrophysical Phenomena and Observations
2016 - IOP Publishing | The Astrophysical Journal
A. Horesh, Chris Stockdale, D. B. Fox, D. A. Frail, John M. Carpenter, S. R. Kulkarni, E. O. Ofek, A. Gal‐Yam, M. M. Kasliwal, I. Arcavi, R. Quimby, S. B. Cenko, P. Nugent, J. S. Bloom, Nicholas M. Law, D. Poznanski, E. Gorbikov, David Polishook, O. Yaron, S. D. Ryder, K. W. Weiler, F. E. Bauer, Schuyler D. Van Dyk, S. Immler, N. Panagia, D. Pooley, N. E. Kassim,
... its surroundings. Our analysis shows that the expanding supernova shockwave does not exhibit equipartition (e_e/e_B ~ ...
Tópico(s): Pulsars and Gravitational Waves Research
2013 - Oxford University Press | Monthly Notices of the Royal Astronomical Society
M. Ackermann, M. Ajello, A. Allafort, L. Baldini, J. Ballet, G. Barbiellini, D. Bastieri, A. Belfiore, R. Bellazzini, B. Berenji, R. D. Blandford, E. D. Bloom, E. Bonamente, A. W. Borgland, E. Bottacini, M. Brigida, Pascal Bruel, R. Buehler, S. Buson, G. A. Caliandro, R. A. Cameron, P. A. Caraveo, J. M. Casandjian, C. Cecchi, A. Chekhtman, C. C. Cheung, J. Chiang, S. Ciprini, R. Claus, J. Cohen-Tanugi, A. De Angelis, F. de Palma, C. D. Dermer, E. do Couto e Silva, P. S. Drell, D. Dumora, C. Favuzzi, S. Fegan, W. B. Focke, P. Fortin, Y. Fukazawa, P. Fusco, F. Gargano, S. Germani, N. Giglietto, F. Giordano, M. Giroletti, T. Glanzman, G. Godfrey, I. A. Grenier, L. Guillemot, S. Guiriec, D. Hadasch, Y. Hanabata, A. K. Harding, M. Hayashida, K. Hayashi, E. Hays, G. Jóhannesson, A. S. Johnson, T. Kamae, H. Katagiri, J. Kataoka, M. Kerr, J. Knödlseder, M. Kuss, J. Landé, L. Latronico, S.-H. Lee, F. Longo, F. Loparco, B. Lott, M. N. Lovellette, P. Lubrano, Pierrick Martin, M. N. Mazziotta, J. E. McEnery, J. Méhault, P. F. Michelson, W. Mitthumsiri, Tsunefumi Mizuno, C. Monte, M. E. Monzani, A. Morselli, I. V. Moskalenko, S. Murgia, M. Naumann-Godó, P. L. Nolan, J. P. Norris, E. Nuss, T. Ohsugi, A. Okumura, E. Orlando, J. F. Ormes, Masanori Ozaki, D. Paneque, D. Parent, M. Pesce-Rollins, M. Pierbattista, F. Piron, M. Pohl, Д. А. Прохоров, S. Rainò, R. Rando, M. Razzano, T. Reposeur, S. Ritz, P. M. Saz Parkinson, C. Sgrò, E. J. Siskind, P. D. Smith, P. Spinelli, A. W. Strong, H. Takahashi, T. Tanaka, J. G. Thayer, J. B. Thayer, D. J. Thompson, L. Tibaldo, D. F. Torres, G. Tosti, A. Tramacere, E. Troja, Y. Uchiyama, J. Vandenbroucke, V. Vasileiou, G. Vianello, V. Vitale, A. P. Waite, P. Wang, B. L. Winer, K. S. Wood, Z. Yang, S. Zimmer, S. Bontemps,
... puzzle. Indirect evidence points to their acceleration by supernova shockwaves, but we know little of their escape from ...
Tópico(s): Gamma-ray bursts and supernovae
2011 - American Association for the Advancement of Science | Science
Ankush Mandal, Christoph Federrath, Bastian Körtgen,
... understood. Previous work suggests that compression caused by supernova shockwaves, gravity, or cloud collisions, may drive the turbulence ...
Tópico(s): Solar and Space Plasma Dynamics
2020 - Oxford University Press | Monthly Notices of the Royal Astronomical Society
J. F. Hansen, M. J. Edwards, D. H. Froula, G. Gregori, Aaron Edens, T. Ditmire,
Tópico(s): Laser-Plasma Interactions and Diagnostics
2005 - Springer Science+Business Media | Astrophysics and Space Science
M. I. Krauss, A. M. Soderberg, Laura Chomiuk, B. A. Zauderer, A. Brunthaler, M. F. Bietenholz, Roger A. Chevalier, Claes Fransson, M. P. Rupen,
... by the self-similar propagation of a spherical shockwave, generated as the supernova ejecta interact with the local circumstellar environment. Modeling ...
Tópico(s): Pulsars and Gravitational Waves Research
2012 - IOP Publishing | The Astrophysical Journal Letters
T. Preibisch, F. Schüller, H. Ohlendorf, Stephanie Pekruhl, K. M. Menten, H. Zinnecker,
... of the strongly irradiated clouds and the expected shockwaves of the imminent supernova explosions.
Tópico(s): Astrophysical Phenomena and Observations
2010 - EDP Sciences | Astronomy and Astrophysics
Y. Butt, T. A. Porter, Boaz Katz, Eli Waxman,
... accelerated to high energies in the rapidly expanding shockwaves created by powerful supernova explosions. Yet observational proof of this conjecture is ...
Tópico(s): Neutrino Physics Research
2008 - Oxford University Press | Monthly Notices of the Royal Astronomical Society Letters
Miloš Milosavljević, Christopher C. Lindner, Rong-Feng Shen, Pawan Kumar,
... be transported outward, where it can drive a supernova-like shockwave. Here we suggest that the energy is transported ...
Tópico(s): Pulsars and Gravitational Waves Research
2011 - IOP Publishing | The Astrophysical Journal
Tópico(s): Dark Matter and Cosmic Phenomena
2013 - Nature Portfolio | Nature
Tópico(s): Pulsars and Gravitational Waves Research
1981 - Oxford University Press | Publications of the Astronomical Society of Japan
Jessie C. Buettel, Barry W. Brook, Andrew A. Cole, J. M. Dickey, Emily J. Flies,
... classes, ecological succession as stellar evolution, wildfire as supernova shockwaves, treefall gaps as interstellar clouds). Ecology–astronomy collaborations ...
Tópico(s): Forest Management and Policy
2018 - Wiley | Ecology and Evolution
J. F. Hansen, M. J. Edwards, D. H. Froula, G. Gregori, Aaron Edens, T. Ditmire,
Supernovae launch spherical shocks into the circumstellar medium (CSM). These shocks may interact with both the intergalactic magnetic field (IGM) and local mass accumulations (possibly with their own local magnetic fields). The latter interaction may trigger star formation. The shocks have high Mach numbers and may be radiative. We have created similar shocks in the laboratory by focusing laser pulses onto the tip of a solid pin surrounded by ambient gas; ablated material from the pin rapidly expands ...
Tópico(s): Astrophysical Phenomena and Observations
2005 - American Institute of Physics | AIP conference proceedings
Robert Megargle, Anthony M. Dean,
... from a 10-MHz crystal oscillator as the Shockwave passed between fixed sensors on the shocktube. Three interval counts so obtained were transmitted to a Supernova computer under program control at the end of ...
Tópico(s): Particle Detector Development and Performance
1974 - Taylor & Francis | Instrumentation Science & Technology
Jack Schulte, Maitrayee Bose, Patrick Young, Gregory Vance,
... fast proton capture after being heated by the supernova shockwave. Both 3D models predict 0.3 <?CDATA $\lt {}^{ ... neutron captures initiated by the propagation of the supernova shockwave. Finally, symmetry has a noticeable effect on the ...
Tópico(s): Nuclear physics research studies
2021 - IOP Publishing | The Astrophysical Journal
In 1987, the brightest supernova seen since 1604 appeared in the Large Magellanic Cloud, a satellite galaxy of the Milky Way about 170,000 light years away. Eleven years later, a new light show is beginning, as the shockwave from the explosion hits a mysterious ring of material that surrounds the star. This collision may show us whether the ...
Tópico(s): Gamma-ray bursts and supernovae
1998 - Nature Portfolio | Nature
Yingchao Lu, Fan Guo, Patrick Kilian, Hui Li, Chengkun Huang, Edison Liang,
... energetic wind into the interior of the expanding shockwave of supernova remnant or interstellar medium. At the termination shock ...
Tópico(s): Pulsars and Gravitational Waves Research
2020 - EDP Sciences | EPJ Web of Conferences
... in this image from the European Southern Observatory.Shockwaves from supernova explosions add to the effect, and the intense ...
2011 - Oxford University Press | Astronomy & Geophysics
... in this image from the European Southern Observatory.Shockwaves from supernova explosions add to the effect, and the intense ...
Tópico(s): Planetary Science and Exploration
2011 - Oxford University Press | Astronomy & Geophysics
... using a model which includes the effect of shockwave of supernova explosion in the stochastic process for the star ...
Tópico(s): Theoretical and Computational Physics
2008 - World Scientific | Fractals
Alak Ray, Harita Palani Balaji, Adarsh Raghu, Gururaj A. Wagle,
Abstract When a supernova shockwave launched deep inside the star exits the surface, it probes the circumstellar medium established by prior mass loss from the pre supernova star. The bright electromagnetic display accompanying the shock breakout is influenced by the properties of the star and scripts the ...
Tópico(s): Astrophysics and Star Formation Studies
2021 - Cambridge University Press | Proceedings of the International Astronomical Union
... among the images conjured up by the word “supernova.” Shockwaves pound outwards and turn rocky asteroids into cometary fluff, driving planetary shards from their orbits and showering neighboring star systems with waves of deadly radiation. It’s dramatic stuff. But what really happens inside the blast wave of a supernova, and, more importantly how can we explain all ...
Tópico(s): Gamma-ray bursts and supernovae
2013 - Springer International Publishing | Astronomers' universe
Xun Liu, Yutong Li, Yujun Zhang, Jiayong Zhong, W. D. Zheng, Qi Dong, Min Chen, Gang Zhao, Y. Sakawa, T. Morita, Yasuhiro Kuramitsu, T. Kato, Liming Chen, Xiaoming Lu, J. L., Weimin Wang, Z. M. Sheng, H. Takabe, Y-J Rhee, Yongkun Ding, Shaoen Jiang, S. Y. Liu, Jingwei Zhu, Jie Zhang,
... the high-power Shenguang II laser facility. The shockwaves observed in our experiment are believed to be excited by collisionless mechanisms. The dimensionless parameters calculated with the results suggest that it is possible to scale the observation to the supernova remnants using transformation and similarity criteria.
Tópico(s): Gamma-ray bursts and supernovae
2011 - IOP Publishing | New Journal of Physics
Weili Lin, Xiaofeng Wang, Lin Yan, A. Gal‐Yam, Jun Mo, Thomas G. Brink, A. V. Filippenko, Danfeng Xiang, R. Lunnan, WeiKang Zheng, P. J. Brown, M. M. Kasliwal, C. Fremling, N. Blagorodnova, D. O. Mirzaqulov, Shuhrat A. Ehgamberdiev, Han Lin, Kaicheng Zhang, Jicheng Zhang, Shengyu Yan, Jujia Zhang, Zhihao Chen, Licai Deng, Kun Wang, Lin Xiao, Ling‐Jun Wang,
... helium-core mass of 48–51 M⊙. Superluminous supernova SN 2017egm has a complex light curve that is well modelled by successive collisions of a shockwave with dense circumstellar shells ejected by its massive ...
Tópico(s): Astrophysical Phenomena and Observations
2023 - Nature Portfolio | Nature Astronomy