Greta Guidi
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View article: A Multiline Analysis of the Distribution and Excitation of CS and H<sub>2</sub>CS in the HD 163296 Disk
A Multiline Analysis of the Distribution and Excitation of CS and H<sub>2</sub>CS in the HD 163296 Disk Open
The abundance and distribution of sulfur-bearing molecules in protoplanetary disks directly influence the composition and potential habitability of nascent planets in addition to providing powerful probes of the physical gas conditions in …
View article: The Large Interferometer For Exoplanets (LIFE): a space mission for mid-infrared nulling interferometry
The Large Interferometer For Exoplanets (LIFE): a space mission for mid-infrared nulling interferometry Open
© 2024 Society of Photo-Optical Instrumentation Engineers (SPIE). This is the accepted manuscript version of a conference paper which has been published in final form at https://doi.org/10.1117/12.3019090
View article: A Survey of Protoplanetary Disks Using the Keck/NIRC2 Vortex Coronagraph
A Survey of Protoplanetary Disks Using the Keck/NIRC2 Vortex Coronagraph Open
Recent Atacama Large Millimeter/submillimeter Array (ALMA) observations of protoplanetary disks in the millimeter continuum have shown a variety of radial gaps, cavities, and spiral features. These substructures may be signposts for ongoin…
View article: Dust properties across the Co snowline in the HD 163296 disk from ALMA and VLA observations
Dust properties across the Co snowline in the HD 163296 disk from ALMA and VLA observations Open
Context. To characterize the mechanisms of planet formation it is crucial to investigate the properties and evolution of protoplanetary disks around young stars, where the initial conditions for the growth of planets are set. The high spat…
View article: Distribution of solids in the rings of the HD 163296 disk: a multiwavelength study
Distribution of solids in the rings of the HD 163296 disk: a multiwavelength study Open
Context. Observations at millimeter wavelengths of bright protoplanetary disks have shown the ubiquitous presence of structures such as rings and spirals in the continuum emission. The derivation of the underlying properties of the emittin…
View article: Large Interferometer For Exoplanets (LIFE)
Large Interferometer For Exoplanets (LIFE) Open
Context. One of the long-term goals of exoplanet science is the atmospheric characterization of dozens of small exoplanets in order to understand their diversity and search for habitable worlds and potential biosignatures. Achieving this g…
View article: ALMA multi-wavelength study of the HD 163296 disk: measuring local variations of dust properties
ALMA multi-wavelength study of the HD 163296 disk: measuring local variations of dust properties Open
HD 163296 is a nearby bright protplanetary disk, presenting a ringed-like structure thats has been associated with the presence of forming planets. We obtained new observations of this targets at 2 and 3 mm with ALMA, that allowed us to de…
View article: A dust and gas cavity in the disc around CQ Tau revealed by ALMA
A dust and gas cavity in the disc around CQ Tau revealed by ALMA Open
The combination of high-resolution and sensitivity offered by ALMA is revolutionizing our understanding of protoplanetary discs, as their bulk gas and dust distributions can be studied independently. In this paper we present resolved ALMA …
View article: High-contrast imaging of HD 163296 with the Keck/NIRC2 L′-band vortex coronograph
High-contrast imaging of HD 163296 with the Keck/NIRC2 L′-band vortex coronograph Open
We present observations of the nearby (D$\\sim$100\\,pc) Herbig star HD~163296\ntaken with the vortex coronograph at Keck/NIRC2 in the L' band (3.7~$\\mu$m), to\nsearch for planetary mass companions in the ringed disc surrounding this\npre…
View article: ALMA Survey of Lupus Protoplanetary Disks II: Gas Disk Radii
ALMA Survey of Lupus Protoplanetary Disks II: Gas Disk Radii Open
We present ALMA Band 6 observations of a complete sample of protoplanetary disks in the young (1-3 Myr) Lupus star-forming region, covering the 1.33 mm continuum and the 12CO, 13CO, and C18O J=2-1 lines. The spatial resolution is 0.25 arcs…
View article: From dust to planets: high resolution observations of small-scale structures in evolving protoplanetary disks
From dust to planets: high resolution observations of small-scale structures in evolving protoplanetary disks Open
This thesis work aimed at studying the first stages planet formation, focusing on protoplanetary disks of gas and dust around pre-main sequence stars. During their relatively short life (≥ 5 Million years) disks are expected to give origin…
View article: Physical properties of dusty protoplanetary disks in Lupus: evidence for viscous evolution?
Physical properties of dusty protoplanetary disks in Lupus: evidence for viscous evolution? Open
Context. 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 sensitivity provided by ALMA, measurements of the…
View article: Lupus disks with faint CO isotopologues: low gas/dust or high carbon depletion?
Lupus disks with faint CO isotopologues: low gas/dust or high carbon depletion? Open
Context. An era has started in which gas and dust can be observed independently in protoplanetary disks, thanks to the recent surveys with the Atacama Large Millimeter/sub-millimeter Array (ALMA). The first near-complete high-resolution di…
View article: ALMA SURVEY OF LUPUS PROTOPLANETARY DISKS. I. DUST AND GAS MASSES
ALMA SURVEY OF LUPUS PROTOPLANETARY DISKS. I. DUST AND GAS MASSES Open
We present the first high-resolution sub-millimeter survey of both dust and gas for a large population of protoplanetary disks. Characterizing fundamental properties of protoplanetary disks on a statistical level is critical to understandi…
View article: Evidence for a correlation between mass accretion rates onto young stars and the mass of their protoplanetary disks
Evidence for a correlation between mass accretion rates onto young stars and the mass of their protoplanetary disks Open
A relation between the mass accretion rate onto the central young star and the mass of the surrounding protoplanetary disk has long been theoretically predicted and observationally sought. For the first time, we have accurately and homogen…
View article: Italian Science Case for ALMA Band 2+3
Italian Science Case for ALMA Band 2+3 Open
The Premiale Project "Science and Technology in Italy for the upgraded ALMA Observatory - iALMA" has the goal of strengthening the scientific, technological and industrial Italian contribution to the Atacama Large Millimeter/submillimeter …