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20112026
most citedBrightness Oscillations in Models of Young Binary Systems with Low-Mass Secondary Components

14 citations · 74 across the 15 of their papers we have counts for

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Showing astro-ph.SRShow all

9 papers · 1 filter

astro-ph.SR2026★ 1 cited

Structure of the Stellar Neighborhood of CQ Tau in the Presence of a Companion in an Elongated Orbit

Tatiana Demidova

There are indirect signs of the presence of a companion near the star CQ\,Tau. A period of 10\;years was found in the brightness changes. The image of the disk shows an extensive c…

astro-ph.SR2026★ 1 cited

Simulation of a protoplanetary disk accretion activity due to a collision with a gas stream

Vitaliy Grigoryev, Tatiana Demidova

The consequences of a protoplanetary disk collision with a gas stream are being studied using three-dimensional numerical gas-dynamic simulation. The influence of orbital parameter…

astro-ph.SR2025★ 4 cited

Simulation of the Free Fall of a Gas Stream on a Protoplanetary Disk

Vitaliy Grigoryev, Tatiana Demidova

The problem of the formation of exoplanets in inclined orbits relative to the equatorial plane of the parent star or the main plane of the protoplanetary disk can be solved by intr…

astro-ph.SR2024

Clumpy accretion as a possible reason of prolonged eclipses of UX~Ori type stars

Vladimir Grinin, Tatiana Demidova

The paper proposes a model of deep and prolonged eclipses of young stars of the UX~Ori type. Some of these events continue for decades and existing models cannot explain them. Our…

astro-ph.SR2023★ 12 cited

3-D SPH simulations of the FUOR flares in the clumpy accretion model

Tatiana V. Demidova, Vladimir P. Grinin

One of the early hypotheses about the origin of FUOR outbursts explains them by the fall of gas clumps from the remnants of protostellar clouds onto protoplanetary disks surroundin…

astro-ph.SR2018★ 5 cited

SPH simulations of structures in protoplanetary disks

Tatiana Demidova, Vladimir Grinin

The hydrodynamic models of the protoplanetary disk, which perturbed by the embeded low-mass companion, were calculated by our modification of GADGET-2 code. The cases of circular a…