activity
20112022
most citedSpiral patterns in planetesimal circumbinary disks

45 citations · 122 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2022★ 12 cited

Clumpy accretion in pre-main-sequence stars as a source of perturbations in circumstellar disks

Tatiana V. Demidova, Vladimir P. Grinin

The development of perturbations in the circumstellar disks of pre-main-sequence stars caused by clumpy accretion was investigated. Here we perform 3D hydrodynamical smoothed parti…

astro-ph.EP2019★ 5 cited

Catastrophic events in protoplanetary disks and their observational manifestations

Tatiana V. Demidova, Vladimir P. Grinin

Observations of protoplanetary disks with high angular resolution using an ALMA interferometer showed that ring-shaped structures are often visible in their images, indicating stro…

astro-ph.EP2016★ 24 cited

Three-lane and multi-lane signatures of planets in planetesimal disks

Tatiana V. Demidova, Ivan I. Shevchenko

In massive numerical experiments we show that a planet embedded in a planetesimal disk induces a characteristic multi-lane "planetosignature" representing a pattern of several stel…

astro-ph.EP2015★ 14 cited

Structures in circumbinary disks: Prospects for observability

Jan Philipp Ruge, Sebastian Wolf, Tatiana Demidova +1

During the past decade circumbinary disks have been discovered around various young binary stars. Hydrodynamical calculations indicate that the gravitational interaction between th…

astro-ph.EP2014★ 45 cited

Spiral patterns in planetesimal circumbinary disks

Tatiana V. Demidova, Ivan I. Shevchenko

Planet formation scenarios and the observed planetary dynamics in binaries pose a number of theoretical challenges, especially in what concerns circumbinary planetary systems. We e…

astro-ph.SR2011★ 13 cited

Modulation of Circumstellar Extinction in a Young Binary System with a Low-Mass Companion in a Noncoplanar Orbit

V. P. Grinin, T. V. Demidova, N. Ya. Sotnikova

The cyclic activity model of a young star with the low-mass secondary component (q = M2/M1 <= 0.1) accreting a matter from circumbinary disk is considered. It is assumed that the o…