activity
19972025
most citedPassive irradiated circumstellar disks with an inner hole

798 citations · 9.5k across the 113 of their papers we have counts for

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53 papers · 1 filter

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

Discovery of an Accretion Burst in a Free-Floating Planetary-Mass Object

V. Almendros-Abad, A. Scholz, B. Damian +7

We report the discovery of a long-lasting burst of disk accretion in Cha J11070768-7626326 (Cha 1107-7626), a young, isolated, 5-10 M object. In spectra taken…

astro-ph.SR2025★ 5 cited

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★ 3 cited

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.SR2024

FitteR for Accretion ProPErties of T Tauri stars (FRAPPE): A new approach to use Class III spectra to derive stellar and accretion properties

R. A. B. Claes, J. Campbell-White, C. F. Manara +10

Studies of the stellar and accretion properties of classical T Tauri stars (CTTS) require comparison with photospheric spectral templates. Here we aim at expanding the currently av…

astro-ph.SR2024

Evolution of the relation between the mass accretion rate and the stellar and disk mass from brown dwarfs to stars

V. Almendros-Abad, C. F. Manara, L. Testi +7

The time evolution of the dependence of the mass accretion rate with the stellar mass and the disk mass represents a fundamental way to understand the evolution of protoplanetary d…