Zobrazeno 1 - 10
of 371
pro vyhledávání: '"I MacFadyen"'
Publikováno v:
Journal of Physics: Conference Series. 46:403-407
During the roughly 20 seconds it shines brightest, a gamma-ray burst (GRB) is over a billion times brighter, in electromagnetic radiation, than an ordinary supernova. The key difference is that GRBs emit some appreciable fraction of their kinetic ene
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2384fb40a2a8e6f8d5e242f3064f98b1
https://doi.org/10.1088/1742-6596/46/1/055
https://doi.org/10.1088/1742-6596/46/1/055
Autor:
D.H. Hartmann, A. I. MacFadyen
Publikováno v:
Nuclear Physics B - Proceedings Supplements. 80:135-142
Cosmic gamma-ray bursts now appropriately hold the distinction of being the “largest explosions in the universe”. Their afterglows are often brighter than supernovae, thus often referred to as “hypernovae”. Their kinetic energies may also be
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b93f98e3fa615d8dc827abcb695ec492
https://doi.org/10.1016/s0920-5632(99)00835-x
https://doi.org/10.1016/s0920-5632(99)00835-x
Autor:
Hendrik J. van Eerten, Andrew I. MacFadyen, Weiqun Zhang, J. E. McEnery, J. L. Racusin, N. Gehrels
Publikováno v:
van Eerten, H J, MacFadyen, A I & Zhang, W 2011, Off-axis afterglow light curves from high-resolution hydrodynamical jet simulations . in J E McEnery, J L Racusin & N Gehrels (eds), American Institute of Physics Conference Proceedings : Gamma Ray Bursts, 2010 . American Institute of Physics Conference Series, vol. 1358, pp. 173-176 . https://doi.org/10.1063/1.3621765
Numerical jet simulations serve a valuable role in calculating gamma-ray burst afterglow emission beyond analytical approximations. Here we present the results of high resolution 2D simulations of decelerating relativistic jets performed using the RA
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5e50b2b2389ef2d4fdf72479b91993be
Publikováno v:
British Journal of Cancer
Mutations in p53 do not account for heritable breast cancer: a study in five affected families
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b7a2af4badbfc1f8476ea8fa65f5d750
http://europepmc.org/articles/PMC1971779
http://europepmc.org/articles/PMC1971779
Autor:
Weiqun Zhang, A. I. MacFadyen
Publikováno v:
AIP Conference Proceedings.
Gamma‐ray bursts are ultra‐relativistic explosions resulting in some cases from the death of massive stars. Numerical modeling of these explosions is challenging because of the extreme Lorentz factors (Γ≳100) and the range of length scales enc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ff409a2599c4dbf5f988fc100933d614
https://doi.org/10.1063/1.2141839
https://doi.org/10.1063/1.2141839
Autor:
A. I. MacFadyen
Publikováno v:
AIP Conference Proceedings.
The fate of massive (Mms≳25 M⊙) rotating stars for which the Type-II supernova mechanism fails to launch a strong explosion is studied by means of 1D and 2D hydrodynamical simulations. In the extreme case (Mms≳35 M⊙) a collapsar-a rapidly acc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::be7e3a71a196763afa104e16344f0165
https://doi.org/10.1063/1.1291718
https://doi.org/10.1063/1.1291718
Publikováno v:
AIP Conference Proceedings.
GRBs have redshifts comparable to, perhaps even larger than those of quasars. Indeed, they are the most energetic explosions in the universe, with energies of order M⊙c2. Their host galaxies are faint, but are actively forming stars at rates typica
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::81c82d7ff2273c6a2f7c3fb67be162a9
https://doi.org/10.1063/1.1361617
https://doi.org/10.1063/1.1361617
Publikováno v:
Astrophysical Journal; 11/20/2024, Vol. 976 Issue 1, p1-8, 8p
Autor:
Zhu, Si-Yuan, Tam, Pak-Hin Thomas
Publikováno v:
Astrophysical Journal; 11/20/2024, Vol. 976 Issue 1, p1-16, 16p