activity
20232026
most citedThe impact of rates of reactions with cosmic ray induced photons on chemical composition of protoplanetary discs

7 citations · 16 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.EP2026

The Effect of X-Ray and Accretion Variability on Mid-Infrared Lines in the Young Disk-Bearing Binary DQ Tau

Bayron Portilla-Revelo, Konstantin V. Getman, Ágnes Kóspál +5

A star's radiation field is the main energy source of a planet-forming disk. Stellar photons---from X-rays to optical---are reprocessed in the inner protoplanetary disk enabling mi…

astro-ph.SR2025★ 6 cited

Time-resolved protoplanetary disk physics in DQ Tau with JWST

Á. Kóspál, P. Ábrahám, V. V. Akimkin +17

Accretion variability is ubiquitous in YSOs. While large outbursts may strongly affect the disk, the effects of moderate bursts are less understood. We aim to study the physical re…

astro-ph.EP2025★ 3 cited

Dancing on the Grain: Variety of CO and its isotopologue fluxes as a result of surface chemistry and T Tauri disk properties

L. Zwicky, T. Molyarova, Á. Kóspál +1

At the moment, one of the main ways to infer the disk mass is to use a combination of CO isotopologue line observations. A number of theoretical studies have concluded that CO must…

astro-ph.EP2025★ 7 cited

The impact of rates of reactions with cosmic ray induced photons on chemical composition of protoplanetary discs

L. N. Zwicky, T. S. Molyarova

Cosmic rays and cosmic ray induced photons are vital components of chemical evolution in areas of interstellar medium that are impenetrable by external ultraviolet radiation. Howev…

astro-ph.SR2025

T CrA has a companion: First direct detection of T CrA B with VLTI/MATISSE

J. Varga, A. Matter, F. Millour +21

T CrA is a Herbig Ae-type young star in a complex circumstellar environment; it includes a circumstellar disk, accretion streamers, jets, and outflows. It has long been suspected t…

astro-ph.SR2023

Observational Chemical Signatures of the Past FU Ori Outbursts

Lis Zwicky, Tamara Molyarova, Vitaly Akimkin +4

FU Ori-type stars are young stellar objects (YSOs) experiencing luminosity outbursts by a few orders of magnitude, which last for years. A dozen of FUors are known up…