The Herbig Ae star HD139614 is a group-Ib object, which featureless SED indicates disk flaring and a possible pre-transitional evolutionary stage. We present mid- and near-IR interferometric results collected with MIDI, AMBER and PIONIER with the aim of constraining the spatial structure of the 0.1-10 AU disk region and assess its possible multi-component structure. A two-component disk model composed of an optically thin 2-AU wide inner disk and an outer temperature-gradient disk starting at 5.6 AU reproduces well the observations. This is an additional argument to the idea that group-I HAeBe inner disks could be already in the disk-clearing transient stage. HD139614 will become a prime target for mid-IR interferometric imaging with the se...
We present the first long baseline mid-infrared interferometric observations of the circumstellar di...
Aims. We study the sub-AU-scale circumstellar environment of the Herbig Ae star HD 144432 with near-...
This is the final version. Available from American Astronomical Society via the DOI in this recordWe...
The formation and evolution of a planetary system are intrinsically linked to the evolution of the p...
Spatially resolving the inner dust cavity (or gap) of the so-called (pre-) transitional disks is a k...
International audienceSpatially resolving the inner dust cavity (or gap) of the so-called (pre-)tran...
We present comprehensive models of the Herbig Ae star, HD 142666, which aim to simultaneously explai...
Aims: We present a mid-IR interferometric survey of the circumstellar environment of a specific clas...
Context. Circumstellar disks surrounding young stars are known to be the birthplaces of planetary sy...
Aims. We present a mid-IR interferometric survey of the circumstellar environment of a specific clas...
Astronomy and Astrophysics 586 (2016): A11 Reproduced with permission from Astronomy & AstrophysicsS...
Context. Circumstellar disks are believed to be the birthplace of planets and are expected to dissip...
The structure and composition of circumstellar disks around young stars is one of the areas in which...
Planet formation has been known for many years to be tied to the spatial distribution of gas and dus...
This is the author accepted manuscript. The final version is available from EDP Sciences via the DOI...
We present the first long baseline mid-infrared interferometric observations of the circumstellar di...
Aims. We study the sub-AU-scale circumstellar environment of the Herbig Ae star HD 144432 with near-...
This is the final version. Available from American Astronomical Society via the DOI in this recordWe...
The formation and evolution of a planetary system are intrinsically linked to the evolution of the p...
Spatially resolving the inner dust cavity (or gap) of the so-called (pre-) transitional disks is a k...
International audienceSpatially resolving the inner dust cavity (or gap) of the so-called (pre-)tran...
We present comprehensive models of the Herbig Ae star, HD 142666, which aim to simultaneously explai...
Aims: We present a mid-IR interferometric survey of the circumstellar environment of a specific clas...
Context. Circumstellar disks surrounding young stars are known to be the birthplaces of planetary sy...
Aims. We present a mid-IR interferometric survey of the circumstellar environment of a specific clas...
Astronomy and Astrophysics 586 (2016): A11 Reproduced with permission from Astronomy & AstrophysicsS...
Context. Circumstellar disks are believed to be the birthplace of planets and are expected to dissip...
The structure and composition of circumstellar disks around young stars is one of the areas in which...
Planet formation has been known for many years to be tied to the spatial distribution of gas and dus...
This is the author accepted manuscript. The final version is available from EDP Sciences via the DOI...
We present the first long baseline mid-infrared interferometric observations of the circumstellar di...
Aims. We study the sub-AU-scale circumstellar environment of the Herbig Ae star HD 144432 with near-...
This is the final version. Available from American Astronomical Society via the DOI in this recordWe...