Debris discs
Empty gaps? Depleting annular regions in debris discs by secular resonance with a two planet system
... In this paper, we will consider a scenario in which there are multiple planets interior to the disc (i.e. within 30au), sculpting the disc via their secular resonances – these reso- nances are important for understanding ...
22
An unbiased study of debris discs around A type stars with Herschel
... the DEBRIS targets, 38 Ari (A077A, HD 17093), was found to have an excess at 160 µ m ...on DEBRIS and SCUBA-2 (Submillimetre Common-User Bolometer Array) data, Pani´c et ...18 debris systems are ...
16
Resolving debris discs in the far-infrared: early highlights from the DEBRIS survey [Letter to the editor]
... of DEBRIS, a Herschel key programme to conduct a volume- and flux-limited survey for debris discs in A-type through M-type ...about discs as close as 11 pc with sizes comparable to that of the ...
5
The Solar System in perspective : from debris discs to extrasolar planets
... of debris discs around FGK stars can be attributed to collisional grinding of ...the discs for each of these ...of discs around later-type stars may be somewhat different from those around ...
154
A statistically significant lack of debris discs in medium separation binary systems
... a debris disc. While nine of the discs appear to be unstable to perturbations from their host binary based on a simple analysis of their inferred radii, we argue that the evidence for genuine instability is ...
22
The gaseous component to planetary debris discs at white dwarfs
... gaseous debris disc around SDSS J1043+0855 was discovered by Gänsicke et ...the debris detected in the photosphere of SDSS J1043+0855, place upper limits on O and Fe, and derive an accretion rate of ...
189
Incidence of debris discs around FGK stars in the solar neighbourhood
... of debris discs, with fundamental contributions from space astronomy in the mid- and far-infrared (λ & 10 µm) since the pioneering dis- covery of an infrared excess in the spectral energy distribution ...
31
Atomic gas in debris discs
... Debris discs represent the final stage of the planet formation pro- ...few debris discs show the presence of small amounts of circumstellar ...
13
An unbiased study of debris discs around A-type stars with Herschel
... of debris discs is typically expected to depend on the spectral type of their host stars as a result of the discs de- tectability being a function of the spectral type (Wyatt 2008) and the ...
16
The grain dynamics and structures of debris discs
... scenario, debris discs are constructed at the time when planetesimals are forming and colliding ...Thus, debris discs can be generated only when there are km-sized planetesimals colliding and ...
5
SONS: The JCMT legacy survey of debris discs in the submillimetre
... detected debris disc based on the observations carried out in this sur- ...known debris discs from Herschel observations, but were too faint to be detected at 850 µm based on the current obser- ...a ...
62
Mass transfer between debris discs during close stellar encounters
... determine the dynamics of the discs. The dust grains are heated by the central star and they re-radiate in the infrared (IR), produc- ing so-called IR excess in the spectral energy distribution of their host star, ...
18
Kuiper belt analogues in nearby M type planet host systems
... the discs and the layout of the planets that orbit closer in, but in each case there remains room in the detection space for sizeable planets that reside between the known planets and the disc, but that could not ...
9
The environments in which stars and circumstellar discs form
... whereas debris discs are composed of recycled material from comet collisions much later in the evolution of the host star, the physics governing the emission of radiation and their detection is essentially ...
180
Discovery of the Fomalhaut C debris disc
... the discs around Fomalhaut and LP 876 − 10 is ...bright debris discs should be no different to random single stars, and their detection in the Fomal- haut system would be attributed to the relative ...
5
Review of State of Art and Process Parameter Influence in EDM Technology
... EDM debris [44].They finalized that the electrical debris particles are present in all sides of components and it does not depend upon the discharge ...
9
Imaging diagnostics for transitional discs
... Transitional discs are a special type of protoplanetary disc, where planet formation is thought to be taking place. These objects feature characteristic inner cavities and/or gaps of a few tens of AUs in ...
13
Chitosan- A Biological Alternative To Chemical Denture Cleansers
... So, the present study aimed to compare and evaluate the efficacy of different concentrations of low molecular weight chitosan and a commercial denture cleanser on the candidal biofilm formed on the dentures. Polymethyl ...
9
EDDA 2.0: integrated simulation of debris flow initiation and dynamics considering two initiation mechanisms
... types of hazards can also interact with each other (e.g. sev- eral small debris flows from sub-channels can merge into a larger one). Therefore, hazard risk assessment requires hy- drological, landslide, and ...
16
Aerodynamic performance of flying discs
... Golf discs can be categorised into three types: ‘putter’, ‘mid-range’ and ‘driver’ discs, each associated with its short (<50 m), medium and long (>75 m) flight range, ...
18