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20192025
most citedSpectral evolution and radial dust transport in the prototype young eruptive system EX Lup

21 citations · 27 across the 5 of their papers we have counts for

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6 papers · 1 filter

astro-ph.SR2025

An interferometric mid-infrared study of the eruptive star binary Z CMa with MATISSE/VLTI. I. Imaging the protoplanetary disks during the 2023 outburst

F. Lykou, J. Varga, F. Cruz-Saénz de Miera +14

The mid-infrared (MIR) emitting regions of the individual protoplanetary disks in the binary system Z CMa are resolved by MATISSE/VLTI. The observations were obtained during a sere…

astro-ph.SR20256 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.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.SR2024

Mid-infrared evidence for iron-rich dust in the multi-ringed inner disk of HD 144432

J. Varga, L. B. F. M. Waters, M. Hogerheijde +40

Context. Rocky planets form by the concentration of solid particles in the inner few au regions of planet-forming disks. Their chemical composition reflects the materials in the di…

astro-ph.SR2023

The disk of the eruptive protostar V900 Mon; a MATISSE/VLTI and MUSE/VLT perspective

F. Lykou, P. Ábrahám, F. Cruz-Sáenz de Miera +8

In this work, we study the silicate dust content in the disk of one of the youngest eruptive stars, V900 Mon, at the highest angular resolution probing down to the inner 10 au of s…

astro-ph.SR201921 cited

Spectral evolution and radial dust transport in the prototype young eruptive system EX Lup

Péter Ábrahám, Lei Chen, Ágnes Kóspál +7

EX Lup is the prototype of a class of pre-main sequence eruptive stars defined by their repetitive outbursts lasting several months. In 2008 January-September EX Lup underwent its…