Inner dusty regions of protoplanetary discs–III. The role of non-radial radiation pressure in dust dynamics
D Vinković, M Čemeljić - Monthly Notices of the Royal …, 2024 - academic.oup.com
We explore the dynamical behaviour of dust particles that populate the surface of inner
optically thick protoplanetary discs. This is a disc region with the hottest dust and is of a great …
optically thick protoplanetary discs. This is a disc region with the hottest dust and is of a great …
Super-Eddington Magnetized Neutron Star Accretion Flows: A Self-similar Analysis
K Chen, ZG Dai - The Astrophysical Journal, 2024 - iopscience.iop.org
The properties of super-Eddington accretion disks exhibit substantial distinctions from the
sub-Eddington ones. In this paper, we investigate the accretion process of a magnetized …
sub-Eddington ones. In this paper, we investigate the accretion process of a magnetized …
2.5-MHD models of circumstellar discs around FS CMa post-mergers: II. Stationary accretion stage
A Moranchel-Basurto, D Korčáková… - Monthly Notices of the …, 2024 - academic.oup.com
We study the star–disc interaction in the presence of the strong magnetic field (B⋆= 6.2 kG)
of a slowly rotating star. This situation describes a post-merger of the spectral type B and has …
of a slowly rotating star. This situation describes a post-merger of the spectral type B and has …
[PDF][PDF] Simulated outflows from accreting magnetized white dwarfs
M Čemeljić, W Kluźniak - tiara.sinica.edu.tw
Results: Qualitatively the results with β-ansatz, shown in Fig. 1 appear similar to the ones
wih α-ansatz from our previous works, but with one interesting additional feature: extremely …
wih α-ansatz from our previous works, but with one interesting additional feature: extremely …