The survey allows us to address some qu... ▽
More Debris discs are a consequence of the planet formation process and constitute the fingerprints of planetesimal systems.
The full sample of 177 FGK stars with d < 20 pc proposed for the DUNES su... ▽
More Debris discs are a consequence of the planet formation process and constitute the fingerprints of planetesimal systems.
Using the HIgh Precision Polarimetric Instrument (H... ▽
More Debris discs are typically revealed through excess emission at infrared wavelengths.
«Over the next few years, I'm optimistic that GPI will reveal many
more debris discs and young planets.
Not exact matches
There, by exploring a very b... ▽
More We present an analysis of the
debris disc around the nearby K2 V star HIP 17439.
The majority of these systems are unresolved and analysis of the dust properties is limited by the lack of information regarding the dust location.vThe Herschel DUNES key program is observing 133 nearby, Sun - like stars (< 20 pc, FGK spectral type) in a volume... ▽
More Dusty
debris discs around main sequence stars are thought to be the result of continuous collisional grinding of planetesimals in the system.
The
discs are found to be well aligned with the stellar equators, as in the case... ▽
More Many nearby main - sequence stars have been searched for
debris using the far - infrared Herschel satellite, within the DEBRIS, DUNES and Guaranteed - Time Key Pro
debris using the far - infrared Herschel satellite, within the
DEBRIS, DUNES and Guaranteed - Time Key Pro
DEBRIS, DUNES and Guaranteed - Time Key Projects.
Our models are compared to a suite of observational data for thermal and scattered light emission, ranging from th... ▽
More The spatially resolved AU Mic
debris disc is among the most famous and best - studied
debris discs.