Zobrazeno 1 - 10
of 59
pro vyhledávání: '"Ruben Krasnopolsky"'
Publikováno v:
The Astrophysical Journal, Vol 965, Iss 1, p 50 (2024)
Using general relativistic magnetohydrodynamic simulations, it has been suggested that the rotational energy of a rapidly rotating black hole (BH) is preferentially extracted along the magnetic field lines threading the event horizon in the middle an
Externí odkaz:
https://doaj.org/article/98cf1d1952c240b9869759477af8e266
Publikováno v:
The Astrophysical Journal, Vol 964, Iss 2, p 147 (2024)
The young stellar source HH 30 is a textbook example of an ionic optical jet originating from a disk in an edge-on system shown by the Hubble Space Telescope. It has a remnant envelope in ^12 CO observed by the Atacama Large Millimeter/submillimeter
Externí odkaz:
https://doaj.org/article/adeb4cf5890d4f4099fbecbd21d64fcc
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 270, Iss 2, p 19 (2024)
Astrochemical simulations are a powerful tool for revealing chemical evolution in the interstellar medium. Astrochemical calculations require efficient processing of large matrices for the chemical networks. The large chemical reaction networks often
Externí odkaz:
https://doaj.org/article/b749289065f045f58b308eecc13bfe48
Publikováno v:
The Astrophysical Journal Letters, Vol 945, Iss 1, p L1 (2023)
We explore a new, efficient mechanism that can power toroidally magnetized jets up to two to three times their original terminal velocity after they enter a self-similar phase of magnetic acceleration. Underneath the elongated outflow lobe formed by
Externí odkaz:
https://doaj.org/article/915931abd62f4d8ca99557226d11e653
Publikováno v:
The Astrophysical Journal, Vol 959, Iss 1, p 32 (2023)
Pseudodisks are dense structures formed perpendicular to the direction of the magnetic field during the gravitational collapse of a molecular cloud core. Numerical simulations of the formation of pseudodisks are usually computationally expensive with
Externí odkaz:
https://doaj.org/article/6928911ac2cd476baaaafd541361e048
Publikováno v:
The Astrophysical Journal, Vol 944, Iss 2, p 230 (2023)
Kinematic signatures of the jet, winds, multicavities, and episodic shells arising in the unified model of bipolar outflows developed in Shang et al. (Paper I), in which an outflow forms by radially directed, wide-angle toroidally magnetized winds in
Externí odkaz:
https://doaj.org/article/24fcfbc1bb3a422687c6a768b8b0f934
Publikováno v:
The Astrophysical Journal, Vol 943, Iss 2, p 164 (2023)
We examine the temporary evolution of axisymmetric magnetospheres around rapidly rotating black holes (BHs), by applying our two-dimensional particle-in-cell simulation code. Assuming a stellar-mass BH, we find that the created pairs fail to screen t
Externí odkaz:
https://doaj.org/article/c97ae73ad9f445d1b3bd8a2c9b702848
We examine the temporary evolution of axisymmetric magnetospheres around rapidly rotating black holes (BHs), by applying our two-dimensional particle-in-cell simulation code. Assuming a stellar-mass BH, we find that the created pairs fail to screen t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9be0c711985c673f0bd6eee07b2dfe5a
http://arxiv.org/abs/2209.13140
http://arxiv.org/abs/2209.13140
Autor:
Ruben Krasnopolsky, Zhi-Yun Li, Ka Ho Lam, Miikka Väisälä, Hsien Shang, Feng Yuan, Weixiao Wang
Misalignment between rotation and magnetic field has been suggested to be one type of physical mechanisms which can easen the effects of magnetic braking during collapse of cloud cores leading to formation of protostellar disks. However, its essentia
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::012e8ca37e0a1936fb04a127f1a98af3
The formation of rings and gaps in wind-launching non-ideal MHD discs: three-dimensional simulations
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 484:107-124
Previous axisymmetric investigations in two dimensions (2D) have shown that rings and gaps develop naturally in non-ideal magnetohydrodynamic (MHD) disk-wind systems, especially in the presence of ambipolar diffusion (AD). Here we extend these 2D sim
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d5720fb28533ca3424722fdcb516a179
https://doi.org/10.1093/mnras/sty3502
https://doi.org/10.1093/mnras/sty3502