11 citations · 29 across the 6 of their papers we have counts for
6 papers
Encounters of star clusters as a possible source of disturbances in their internal structure
M. D. Sizova, L. A. Maksimova, S. V. Vereshchagin
We searched for past close encounters of the Hyades and Pleiades with all 5736 clusters of the Hunt & Reffert catalog, integrating orbits with galpy over the last 100 Myr and valid…
Simulation of Thermal Surface Waves in a Protoplanetary Disk in a Two-Dimensional Approximation
Ya. N. Pavlyuchenkov, L. A. Maksimova, V. V. Akimkin
Theoretical models predict that the obscuration of stellar radiation by irregularities on the surface of a protoplanetary disk can cause self-generating waves traveling towards the…
Simulations of thermal surface waves in a protoplanetary disk using 1+1D approximation
Ya. N. Pavlyuchenkov, L. A. Maksimova, V. V. Akimkin
Heating by the central star is one of the key factors determining the physical structure of protoplanetary disks. Due to the large optical thickness in the radial direction, disk m…
Evolution of a Viscous Protoplanetary Disk with Convectively Unstable Regions. II. Accretion Regimes and Long-Term Dynamics
L. A. Maksimova, Ya. N. Pavlyuchenkov, A. V. Tutukov
In this article, we proceed to study convection as a possible factor of episodic accretion in protoplanetary disks. Within the model presented in Article~I, the accretion history i…
Evolution of a Viscous Protoplanetary Disk with Convectively Unstable Regions
Ya. N. Pavlyuchenkov, A. V. Tutukov, L. A. Maksimova +1
The role of convection in the gas-dust accretion disk around a young star is studied. The evolution of a Keplerian disk is modeled using the Pringle equation, which describes the t…
Astrometric observations of outer Jovian satellites with the `Saturn' telescope. First results
M. Yu. Khovritchev, A. P. Ershova, I. A. Balyaev +9
The one-meter telescope-reflector `Saturn' (D=1 m, F = 4 m) was partially renovated at the Pulkovo observatory at the end of 2014. The telescope was equipped by CCD camera S2C with…