82 citations · 268 across the 6 of their papers we have counts for
6 papers
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…
A giant planet shaping the disk around the very low-mass star CIDA 1
P. Curone, A. F. Izquierdo, L. Testi +13
(Abridged) Exoplanetary research has provided us with exciting discoveries of planets around very low-mass (VLM) stars (e.g., TRAPPIST-1 and Proxima Centauri). However, current the…
The protoplanetary disk population in the rho-Ophiuchi region L1688 and the time evolution of Class II YSOs
L. Testi, A. Natta, C. F. Manara +10
(Abridged) We present a study of the disk population in L1688, the densest and youngest region in Ophiuchus, and we compare it with other nearby regions of different age, namely Lu…
PENELLOPE: the ESO data legacy program to complement the Hubble UV Legacy Library of Young Stars (ULLYSES) I. Survey presentation and accretion properties of Orion OB1 and -Orionis
C. F. Manara, A. Frasca, L. Venuti +69
The evolution of young stars and disks is driven by the interplay of several processes, notably accretion and ejection of material. Critical to correctly describe the conditions of…
A bright inner disk and structures in the transition disk around the very low-mass star CIDA 1
P. Pinilla, N. T. Kurtovic, M. Benisty +7
Observations of protoplanetary disks around very low-mass stars and brown dwarfs remain challenging and little is known about their properties. The disk around CIDA1 (0.1-0.2…
Measuring the ratio of the gas and dust emission radii of protoplanetary disks in the Lupus star-forming region
E. Sanchis, L. Testi, A. Natta +15
We perform a comprehensive demographic study of the CO extent relative to dust of the disk population in the Lupus clouds, in order to find indications of dust evolution and possib…