Results 11 to 20 of about 7,087 (197)
The Debris Disk Explorer: a balloon-borne coronagraph for observing debris disks [PDF]
13 pages, 8 figures.
Wesley Traub +2 more
exaly +5 more sources
MOLECULAR GAS IN YOUNG DEBRIS DISKS [PDF]
Accepted for publication in ApJ Letters, 8 pages, 3 figures, 1 tables (emulateapj style)
A Moor, P Abraham, Ilaria Pascucci
exaly +4 more sources
ON THE RELATIONSHIP BETWEEN DEBRIS DISKS AND PLANETS [PDF]
Dust in debris disks is generated by collisions among planetesimals. The existence of these planetesimals is a consequence of the planet formation process, but the relationship between debris disks and planets has not been clearly established. Here we analyze Spitzer/MIPS 24 and 70 micrometer data for 150 planet-bearing stars, and compare the incidence
A Kóspál, David Ardila, Attila Moor
exaly +5 more sources
The Study of Debris Disks with SPICA [PDF]
Debris disks are evidence that stars harbor reservoirs of dust-producing plantesimals on spatial scales similar the solar system. Debris disks present a wide range of sizes and structural features and there is growing evidence that, in some cases, they might be the result of the dynamical perturbations of a massive planet. Our solar system also harbors
Amaya Moro-Martίn
openaire +3 more sources
A search for debris disks in theHerschel-ATLAS [PDF]
5 pages, 3 figures, accepted by A&A for the Herschel Special ...
Thompson, M. A. +45 more
core +14 more sources
Review chapter of the book "Planetary Systems Now", to be published by World ...
Sebastian Marino
exaly +3 more sources
Observing planet-disk interaction in debris disks [PDF]
Context. Structures in debris disks induced by planetdisk interaction are promising to provide valuable constraints on the existence and properties of embedded planets. Aims. We investigate the observability of structures in debris disks induced by planet-disk interaction. Methods.
Ertel, S., Wolf, S., Rodmann, J.
openaire +6 more sources
Debris disks around M dwarfs: The Herschel DEBRIS survey [PDF]
The Herschel open-time key program Disc Emission via a Bias-free Reconnaissance in the Infrared and Sub-millimeter (DEBRIS) is an unbiased survey of the nearest ∼100 stars for each stellar type A-M observed with a uniform photometric sensitivity to search for cold debris disks around them.
Lestrade, J.-F. +9 more
openaire +5 more sources
Secret of Longevity: Protoplanetary Disks as a Source of Gas in Debris Disks [PDF]
While protoplanetary disks (PPDs) are generally thought to disperse within several million years, recent observations have revealed gas in their older counterparts, debris disks.
Wataru Ooyama +4 more
doaj +2 more sources
A Constraint on the Amount of Hydrogen from the CO Chemistry in Debris Disks
The faint CO gases in debris disks are easily dissolved into C by UV irradiation, while CO can be reformed via reactions with hydrogen. The abundance ratio of C/CO could thus be a probe of the amount of hydrogen in the debris disks.
Kazunari Iwasaki +3 more
doaj +1 more source

