activity
20172022
most citedRetrieving scattering clouds and disequilibrium chemistry in the atmosphere of HR 8799e

221 citations · 345 across the 6 of their papers we have counts for

collaborators

7 papers

astro-ph.EP202213 cited

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…

astro-ph.EP202121 cited

Gravitoviscous protoplanetary disks with a dust component. V. The dynamic model for freeze-out and sublimation of volatiles

Tamara Molyarova, Eduard I. Vorobyov, Vitaly Akimkin +3

The snowlines of various volatile species in protoplanetary disks are associated with abrupt changes in gas composition and dust physical properties. Volatiles may affect dust grow…

astro-ph.EP2020221 cited

Retrieving scattering clouds and disequilibrium chemistry in the atmosphere of HR 8799e

P. Mollière, T. Stolker, S. Lacour +25

Clouds are ubiquitous in exoplanet atmospheres and represent a challenge for the model interpretation of their spectra. Complex cloud models are too numerically costly for generati…

astro-ph.EP2020

Chemical modelling of FU Ori protoplanetary disks

Tamara Molyarova, Vitaly Akimkin, Dmitry Semenov +5

Luminosity outbursts of the FUOri type stars, which have a magnitude of and last for decades, may affect chemical composition of the surrounding protoplanetary…

astro-ph.EP201944 cited

Luminosity outburst chemistry in protoplanetary discs: going beyond standard tracers

Dmitri S. Wiebe, Tamara S. Molyarova, Vitaly V. Akimkin +2

The chemical influence of luminosity outbursts on the environments of young solar-type stars is explored. Species are categorised into several types according to their response to…

astro-ph.EP2018

Chemical Signatures of the FU Ori Outbursts

Tamara Molyarova, Vitaly Akimkin, Dmitry Semenov +5

The FU Ori-type young stellar objects are characterized by a sudden increase in luminosity by 12 orders of magnitude, followed by slow return to the pre-outburst state on timesc…