379 citations · 700 across the 11 of their papers we have counts for
10 papers
Mid-infrared blends and continuum signatures of dust drift and accretion in protoplanetary disks
S. Antonellini, I. Kamp, L. B. F. M Waters
The MIR blend fluxes correlation between HCN and water can be explained as a consequence of dust evolution, namely, changes in the dust MIR opacity. Other disk properties, such as…
Fevering Interstellar Ices Have More CH3OD
Beatrice M. Kulterer, Maria N. Drozdovskaya, Stefano Antonellini +2
Mono-deuterated methanol is thought to form during the prestellar core stage of star formation. Observed variations in the CH2DOH/CH3OD ratio suggest that its formation is strongly…
A model exploration of NIR ro-vibrational CO emission as a tracer of inner cavities in protoplanetary disks
S. Antonellini, A. Banzatti, I. Kamp +2
Near-IR observations of protoplanetary disks provide information about the properties of the inner disk. High resolution spectra of abundant molecules such as CO can be used to det…
Consistent dust and gas models for protoplanetary disks IV. A panchromatic view of protoplanetary disks
O. Dionatos, P. Woitke, M. Guedel +17
Consistent modeling of protoplanetary disks requires the simultaneous solution of both continuum and line radiative transfer, heating/cooling balance between dust and gas and, of c…
Consistent dust and gas models for protoplanetary disks III. Models for selected objects from the FP7 DIANA project
P. Woitke, I. Kamp, S. Antonellini +17
The European FP7 project DIANA has performed a coherent analysis of a large set of observations from protoplanetary disks by means of thermo-chemical disk models. The collected dat…
Multi-wavelength observations of planet forming disks: Constraints on planet formation processes
Inga Kamp, Stefano Antonellini, Andres Carmona +2
Our understanding of protoplanetary disks has greatly improved over the last decade due to a wealth of data from new facilities. Unbiased dust surveys with Spitzer leave us with go…
The mid-IR water and silicate relation in protoplanetary disks
S. Antonellini, J. Bremer, I. Kamp +7
Mid-IR water lines from protoplanetary disks around T Tauri stars have a detection rate of 50\%. Models have identified multiple physical properties of disks such as dust-to-gas ma…
Consistent dust and gas models for protoplanetary disks. I. Disk shape, dust settling, opacities, and PAHs
P. Woitke, M. Min, C. Pinte +19
We propose a set of standard assumptions for the modelling of Class II and III protoplanetary disks, which includes detailed continuum radiative transfer, thermo-chemical modelling…
Mid-IR spectra of Pre-Main Sequence Herbig stars: an explanation for the non-detections of water lines
S. Antonellini, I. Kamp, F. Lahuis +7
The mid-IR detection rate of water lines in disks around Herbig stars disks is about 5\%, while it is around 50\% for disks around TTauri stars. The reason for this is still unclea…
Understanding the water emission in the mid- and far-IR from protoplanetary disks around T~Tauri stars
S. Antonellini, I. Kamp, P. Riviere-Marichalar +6
We investigate which properties of protoplanetary disks around T Tauri stars affect the physics and chemistry in the regions where mid- and far-IR water lines originate and their r…