most citedVLTI images of circumbinary disks around evolved stars

3 citations · 4 across the 4 of their papers we have counts for

collaborators

9 papers

astro-ph.SR2025

The dance of dust: Investigating young stellar object dipper variability

A. Empey, R. Garcia Lopez, A. Natta +4

The dipper subclass of YSOs are characterised by frequent dips in their light curves. Irregular dippers do not show periodic signatures and have dips accounting for significant pro…

astro-ph.SR2025

PENELLOPE VII: Revisiting empirical relations to measure accretion luminosity

E. Fiorellino, J. M. Alcalá, C. F. Manara +10

The accretion luminosity (Lacc) in young, low-mass stars is crucial for understanding stellar formation, but direct measurements are often hindered by limited spectral coverage and…

astro-ph.SR2025

Probing accretion and stellar properties in the Orion Nebula with VLT/X-Shooter

L. Piscarreta, G. Beccari, R. A. B. Claes +6

Multiple photometric studies have reported the presence of seemingly older accreting pre-main sequence stars (PMS) in optical colour-magnitude diagrams (CMDs). We investigate this…

astro-ph.SR2025

The ODYSSEUS Survey. Characterizing magnetospheric geometries and hotspot structures in T Tauri stars

Caeley V. Pittman, C. C. Espaillat, Connor E. Robinson +20

Magnetospheric accretion is a key process that shapes the inner disks of T Tauri stars, controlling mass and angular momentum evolution. It produces strong ultraviolet and optical…

astro-ph.SR2025

The accretion luminosity of Class I protostars

L. Testi, A. Natta, S. Gozzi +7

The value of the accretion luminosity during the early phases of star formation is a crucial information which helps us understand how stars form, yet it is still very difficult to…

astro-ph.EP2025

Disk Evolution Study Through Imaging of Nearby Young Stars (DESTINYS): Evidence of planet-disk interaction in the 2MASSJ16120668-3010270 system

C. Ginski, P. Pinilla, M. Benisty +28

The architectures of exoplanet systems are likely set during the initial planet-formation phase in the circumstellar disk. To understand this process, we have to study the earliest…