Zobrazeno 1 - 10
of 55
pro vyhledávání: '"Shigenobu Hirose"'
Autor:
Sebastian Baum, Patrick Stengel, Natsue Abe, Javier F. Acevedo, Gabriela R. Araujo, Yoshihiro Asahara, Frank Avignone, Levente Balogh, Laura Baudis, Yilda Boukhtouchen, Joseph Bramante, Pieter Alexander Breur, Lorenzo Caccianiga, Francesco Capozzi, Juan I. Collar, Reza Ebadi, Thomas Edwards, Klaus Eitel, Alexey Elykov, Rodney C. Ewing, Katherine Freese, Audrey Fung, Claudio Galelli, Ulrich A. Glasmacher, Arianna Gleason, Noriko Hasebe, Shigenobu Hirose, Shunsaku Horiuchi, Yasushi Hoshino, Patrick Huber, Yuki Ido, Yohei Igami, Norito Ishikawa, Yoshitaka Itow, Takashi Kamiyama, Takenori Kato, Bradley J. Kavanagh, Yoji Kawamura, Shingo Kazama, Christopher J. Kenney, Ben Kilminster, Yui Kouketsu, Yukiko Kozaka, Noah A. Kurinsky, Matthew Leybourne, Thalles Lucas, William F. McDonough, Mason C. Marshall, Jose Maria Mateos, Anubhav Mathur, Katsuyoshi Michibayashi, Sharlotte Mkhonto, Kohta Murase, Tatsuhiro Naka, Kenji Oguni, Surjeet Rajendran, Hitoshi Sakane, Paola Sala, Kate Scholberg, Ingrida Semenec, Takuya Shiraishi, Joshua Spitz, Kai Sun, Katsuhiko Suzuki, Erwin H. Tanin, Aaron Vincent, Nikita Vladimirov, Ronald L. Walsworth, Hiroko Watanabe
Minerals are solid state nuclear track detectors - nuclear recoils in a mineral leave latent damage to the crystal structure. Depending on the mineral and its temperature, the damage features are retained in the material from minutes (in low-melting
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::39661f426cd2f86bd735040b6a3d8100
Autor:
Shigenobu Hirose, Ji-Ming Shi
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 485:266-285
Using local three dimensional radiation hydrodynamics simulations, the nonlinear outcome of gravitational instability in an irradiated protoplanetary disc is investigated in a parameter space of the surface density $\Sigma$ and the radius $r$. Starti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9e04bd959ec491f04326cf8cefe25bd4
https://doi.org/10.1093/mnras/stz163
https://doi.org/10.1093/mnras/stz163
Publikováno v:
Astronomy & Astrophysics. 659:A87
We have developed a public code, Optab, that outputs Rosseland, Planck, and two-temperature Planck mean gas opacity tables for radiation hydrodynamics simulations in astrophysics. The code is developed for modern high-performance computing, being wri
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::78b4faeb6d2ab6bb094742b2271a5cef
https://doi.org/10.1051/0004-6361/202141076
https://doi.org/10.1051/0004-6361/202141076
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 462:3710-3726
The phenomenological Disc Instability Model has been successful in reproducing the observed light curves of dwarf nova outbursts by invoking an enhanced Shakura-Sunyaev $\alpha$ parameter $\sim0.1-0.2$ in outburst compared to a low value $\sim0.01$ i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5fa8c8e16b7de5168b8e78d28678eb1f
https://doi.org/10.1093/mnras/stw1908
https://doi.org/10.1093/mnras/stw1908
Warm Comptonization models for the soft X-ray excess in AGN do not self-consistently explain the relationship between the Comptonizing medium and the underlying accretion disc. Because of this, they cannot directly connect the fitted Comptonization t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8b596927ecd7f37a9e1881f76993aca0
We present the results of local, vertically stratified, radiation magnetohydrodynamic shearing box simulations of magnetorotational instability (MRI) turbulence for a (hydrogen poor) composition applicable to accretion disks in AM CVn type systems. M
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ff0e44d09cf79d8270128c066291f944
Autor:
Shigenobu Hirose
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 448:3105-3120
Using radiation magnetohydrodynamics simulations with realistic opacities and equation of state, and zero net magnetic flux, we have explored thermodynamics in the inner part of protoplanetary discs where magnetic turbulence is expected. The thermal
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2f4b571572a55fb0d8714e879985539d
https://doi.org/10.1093/mnras/stv203
https://doi.org/10.1093/mnras/stv203
Autor:
Shigenobu Hirose, Ji-Ming Shi
Using radiation hydrodynamics simulations in a local stratified shearing box with realistic equations of state and opacities, we explored the outcome of self-gravity at 50 AU in a protoplanetary disc irradiated by the central star. We found that grav
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::26fb5ac860ab3f1f73c74206f9383be2
http://arxiv.org/abs/1703.10292
http://arxiv.org/abs/1703.10292
Publikováno v:
The Astrophysical Journal. 708:1716-1727
We study the properties of the turbulence driven by the magnetorotational instability in a stratified shearing box with outflow boundary conditions and an equation of state determined by self-consistent dissipation and radiation losses. A series of s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::03583bb09789b6bcf8ce83b88a0e2931
https://doi.org/10.1088/0004-637x/708/2/1716
https://doi.org/10.1088/0004-637x/708/2/1716
Publikováno v:
The Astrophysical Journal. 704:1065-1085
This article reports on three-dimensional (3-D) MHD simulations of non-rotating and rapidly rotating black holes and the adjacent black hole accretion disk magnetospheres. A particular emphasis is placed on the vertical magnetic flux that is advected
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cfa11c81ad37eeae4fd901a7f8a2de06
https://doi.org/10.1088/0004-637x/704/2/1065
https://doi.org/10.1088/0004-637x/704/2/1065