Ph.D. University of Hawaii at Manoa 2012.Includes bibliographical references.At an age of 1 million years, massive dust and gas rich circumstellar disks are ubiquitous, while by 10 million years most disks have become undetectable. I have focused on the characterization of circumstellar disks in the 5 million year old Upper Scorpius group, a group of stars that probe the middle of this age range, in order to gain insight to the speed at which the disk dissipation process occurs and the time available for giant planet formation. I have carried out the most sensitive survey to-date for millimeter continuum emission from large dust grains in intermediate aged disks. With a dust mass sensitivity of 4x10-3 MJup and under the assumption of the pr...
We characterize the first 40 Myr of evolution of circumstellar disks through a unified study of the ...
We present 4.5, 8, and 16 µm photometry from the Spitzer Space Telescope for 204 stars in the Upper ...
Determining the mechanisms that drive the evolution of protoplanetary disks is a necessary step towa...
International audienceWe present results of far-infrared photometric observations with Herschel PACS...
International audienceWe present results of far-infrared photometric observations with Herschel PACS...
International audienceWe present results of far-infrared photometric observations with Herschel PACS...
Artículo de publicación ISIWe present results of far-infrared photometric observations with Herschel...
Artículo de publicación ISIWe present results of far-infrared photometric observations with Herschel...
We present results of far-infrared photometric observations with Herschel PACS of a sample...
We present results of far-infrared photometric observations with Herschel PACS of a sample...
We present results of far-infrared photometric observations with Herschel PACS of a sample...
We present detailed modeling of the spatial distributions of gas and dust in 57 circumstellar disks ...
Funding: CFM acknowledges an ESO fellowship. This project has received funding from the European Uni...
We have carried out a Spitzer survey for brown dwarf disks in the 5 Myr old Upper Scorpius (UpSco) s...
We present 4.5, 8, and 16 µm photometry from the Spitzer Space Telescope for 204 stars in the Upper ...
We characterize the first 40 Myr of evolution of circumstellar disks through a unified study of the ...
We present 4.5, 8, and 16 µm photometry from the Spitzer Space Telescope for 204 stars in the Upper ...
Determining the mechanisms that drive the evolution of protoplanetary disks is a necessary step towa...
International audienceWe present results of far-infrared photometric observations with Herschel PACS...
International audienceWe present results of far-infrared photometric observations with Herschel PACS...
International audienceWe present results of far-infrared photometric observations with Herschel PACS...
Artículo de publicación ISIWe present results of far-infrared photometric observations with Herschel...
Artículo de publicación ISIWe present results of far-infrared photometric observations with Herschel...
We present results of far-infrared photometric observations with Herschel PACS of a sample...
We present results of far-infrared photometric observations with Herschel PACS of a sample...
We present results of far-infrared photometric observations with Herschel PACS of a sample...
We present detailed modeling of the spatial distributions of gas and dust in 57 circumstellar disks ...
Funding: CFM acknowledges an ESO fellowship. This project has received funding from the European Uni...
We have carried out a Spitzer survey for brown dwarf disks in the 5 Myr old Upper Scorpius (UpSco) s...
We present 4.5, 8, and 16 µm photometry from the Spitzer Space Telescope for 204 stars in the Upper ...
We characterize the first 40 Myr of evolution of circumstellar disks through a unified study of the ...
We present 4.5, 8, and 16 µm photometry from the Spitzer Space Telescope for 204 stars in the Upper ...
Determining the mechanisms that drive the evolution of protoplanetary disks is a necessary step towa...