231 citations · 3k across the 55 of their papers we have counts for
9 papers · 1 filter
The wind and the magnetospheric accretion onto the T Tauri star S Coronae Australis at sub-au resolution
R. Garcia Lopez, K. Perraut, A. Caratti o Garatti +70
To investigate the inner regions of protoplanetary disks, we performed near-infrared interferometric observations of the classical TTauri binary system S CrA. We present the first…
CN rings in full protoplanetary disks around young stars as probes of disk structure
P. Cazzoletti, E. F. van Dishoeck, R. Visser +2
Bright ring-like structure emission of the CN molecule has been observed in protoplanetary disks. We investigate whether such structures are due to the morphology of the disk itsel…
Physical properties of dusty protoplanetary disks in Lupus: evidence for viscous evolution?
M. Tazzari, L. Testi, A. Natta +9
The formation of planets strongly depends on the total amount as well as on the spatial distribution of solids in protoplanetary disks. Thanks to the improvements in resolution and…
NH_3(1_0-0_0) in the pre-stellar core L1544
P. Caselli, L. Bizzocchi, E. Keto +11
Pre-stellar cores represent the initial conditions in the process of star and planet formation, therefore it is important to study their physical and chemical structure. Because of…
Non-thermal photons and direct photodissociation of H2, HD and HeH+ in the chemistry of the primordial Universe
C. M. Coppola, M. V. Kazandjian, D. Galli +2
Non-thermal photons deriving from radiative transitions among the internal ladder of atoms and molecules are an important source of photons in addition to thermal and stellar sourc…
Different dust and gas radial extents in protoplanetary disks: consistent models of grain growth and CO emission
Stefano Facchini, Til Birnstiel, Simon Bruderer +1
ALMA observations of protoplanetary disks confirm earlier indications that there is a clear difference between the dust and gas radial extents. The origin of this difference is sti…