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TYC 8241 2652 1 and the case of the disappearing disk: no smoking gun yet
Hans Moritz Günther, Stefan Kraus, Carl Melis +12
TYC 8241 2652 1 is a young star that showed a strong mid-infrared (mid-IR, 8-25 mu) excess in all observations before 2008 consistent with a dusty disk. Between 2008 and 2010 the m…
Cophasing the Planet Formation Imager
Romain G. Petrov, Abdelkarim Boskri, Thami Elhalkouj +3
The Planet Formation Imager (PFI) is a project for a very large optical interferometer intended to obtain images of the planet formation process at scales as small as the Hill sphe…
The Frequency Of Binary Star Interlopers Amongst Transitional Discs
D. Ruíz-Rodríguez, M. Ireland, L. Cieza +1
Using Non-Redundant Mask interferometry (NRM), we searched for binary companions to objects previously classified as Transitional Disks (TD). These objects are thought to be an evo…
Practical Beam Transport for the Planet Formation Imager (PFI)
David Mozurkewich, John Young, Michael Ireland
The Planet Formation Imager (PFI) is a future kilometric-baseline infrared interferometer to image the complex physical processes of planet formation. Technologies that could be us…
Beam combination schemes and technologies for the Planet Formation Imager (PFI)
Stefano Minardi, Sylvestre Lacour, Jean-Philippe Berger +4
The Planet Formation Imager (PFI) initiative aims at developing the next generation large scale facility for imaging astronomical optical interferometry operating in the mid-infrar…
Status of the Planet Formation Imager (PFI) concept
Michael J. Ireland, John D. Monnier, Stefan Kraus +11
The Planet Formation Imager (PFI) project aims to image the period of planet assembly directly, resolving structures as small as a giant planet's Hill sphere. These images will be…