90 citations · 888 across the 43 of their papers we have counts for
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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…
Efficiency of the top-down PAH-to-fullerene conversion in UV irradiated environments
M. S. Murga, V . V. Akimkin, D. S. Wiebe
Polycyclic aromatic hydrocarbons (PAHs) and fullerenes play a major role in the physics and chemistry of the interstellar medium. Based on a number of recent experimental and theor…
Dust grains cannot grow to millimeter sizes in protostellar envelopes
Kedron Silsbee, Vitaly Akimkin, Alexei V. Ivlev +3
A big question in the field of star and planet formation is the time at which substantial dust grain growth occurs. The observed properties of dust emission across different wavele…
Machine learning-accelerated chemistry modeling of protoplanetary disks
Grigorii V. Smirnov-Pinchukov, Tamara Molyarova, Dmitry A. Semenov +4
Aims. With the large amount of molecular emission data from (sub)millimeter observatories and incoming James Webb Space Telescope infrared spectroscopy, access to fast forward mode…
The Young Binary DQ Tau Produces Another X-ray Flare Near Periastron
Konstantin V. Getman, Vitaly V. Akimkin, Nicole Arulanantham +4
This work is part of a multi-wavelength program to study the effects of X-ray/UV/optical stellar radiation on the chemistry of the circumbinary disk around the young high-eccentric…
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…