Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Moupiya Maji"'
Autor:
Qirong Zhu, Yuexing Li, Yiting Li, Moupiya Maji, Hidenobu Yajima, Raffaella Schneider, Lars Hernquist
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 514:5583-5606
Supermassive black holes (SMBHs) of $\sim 10^9\, \rm M_{\odot }$ are generally believed to be the central engines of the luminous quasars observed at z ≳ 6, but their astrophysical origin remains elusive. To investigate the formation of these dista
Autor:
Moupiya Maji, Anne Verhamme, Joakim Rosdahl, Thibault Garel, Jérémy Blaizot, Valentin Mauerhofer, Marta Pittavino, Maria-Pia Victoria Feser, Mathieu Chuniaud, Taysun Kimm, Harley Katz, Martin Haehnelt
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 663, ⟨10.1051/0004-6361/202142740⟩
Astronomy and Astrophysics-A&A, 2022, 663, ⟨10.1051/0004-6361/202142740⟩
Aims. The primary difficulty in understanding the sources and processes that powered cosmic reionization is that it is not possible to directly probe the ionizing Lyman-continuum (LyC) radiation at that epoch as those photons have been absorbed by th
ART$^2$ is a 3D multi-wavelength Monte Carlo radiative transfer (RT) code that couples continuum and emission lines to track the propagation of photons and their interactions with the interstellar medium (ISM). The previous version of ART$^2$, which
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::77703bab0b1810a05057d468728bd808
http://arxiv.org/abs/2001.11146
http://arxiv.org/abs/2001.11146
The "Disk of satellites" (DoS) around Milky Way is a highly debated topic with conflicting interpretations of observations and their theoretical models. We perform a comprehensive analysis of all dwarfs detected in the Milky Way and find that the DoS
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6fd563d515019e1eb09229ff459a4921
http://hdl.handle.net/11585/663716
http://hdl.handle.net/11585/663716
Observations of globular clusters show that they have universal lognormal mass functions with a characteristic peak at $\sim 2\times 10^{5}\, {\rm{M_{\odot}}}$, but the origin of this peaked distribution is highly debated. Here we investigate the for
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e9f977b9142d6494ba72545b2f755ca3
We study the impact of baryons on the distribution of dark matter in a Milky Way-size halo by comparing a high-resolution, moving-mesh cosmological simulation with its dark matter-only counterpart. We identify three main processes related to baryons
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::94eb33e3dd610d5e8a611bc17b6edbe1
Publikováno v:
Astrophysical Journal; 8/1/2017, Vol. 844 Issue 2, p1-1, 1p
Publikováno v:
Astrophysical Journal; 7/1/2017, Vol. 843 Issue 1, p1-1, 1p