Evolution of debris disks
MC Wyatt - Annu. Rev. Astron. Astrophys., 2008 - annualreviews.org
Circumstellar dust exists around several hundred main sequence stars. For the youngest
stars, that dust could be a remnant of the protoplanetary disk. Mostly it is inferred to be …
stars, that dust could be a remnant of the protoplanetary disk. Mostly it is inferred to be …
The alpha-defensin immunoassay and leukocyte esterase colorimetric strip test for the diagnosis of periprosthetic infection: a systematic review and meta-analysis
MC Wyatt, AD Beswick, SK Kunutsor, MJ Wilson… - JBJS, 2016 - journals.lww.com
Background: Synovial biomarkers have recently been adopted as diagnostic tools for
periprosthetic joint infection (PJI), but their utility is uncertain. The purpose of this systematic …
periprosthetic joint infection (PJI), but their utility is uncertain. The purpose of this systematic …
How observations of circumstellar disk asymmetries can reveal hidden planets: pericenter glow and its application to the HR 4796 disk
MC Wyatt, SF Dermott, CM Telesco… - The Astrophysical …, 1999 - iopscience.iop.org
Recent images of the disks of dust around the young stars HR 4796A and Fomalhaut show,
in each case, a double-lobed feature that may be asymmetric (one lobe may be brighter than …
in each case, a double-lobed feature that may be asymmetric (one lobe may be brighter than …
Custom 3D-printed acetabular implants in hip surgery–innovative breakthrough or expensive bespoke upgrade?
MC Wyatt - Hip International, 2015 - journals.sagepub.com
Custom 3D-printed triflange acetabular cages are a new option in the armamentarium of the
revision hip surgeon. This review article defines this technology, its indications, surgical …
revision hip surgeon. This review article defines this technology, its indications, surgical …
Transience of hot dust around sun-like stars
MC Wyatt, R Smith, JS Greaves… - The Astrophysical …, 2007 - iopscience.iop.org
In this paper a simple model for the steady state evolution of debris disks due to collisions is
developed and confronted with the properties of the emerging population of seven Sun-like …
developed and confronted with the properties of the emerging population of seven Sun-like …
Planet Hunters IX. KIC 8462852–where's the flux?
TS Boyajian, DM LaCourse… - Monthly notices of …, 2016 - academic.oup.com
Over the duration of the Kepler mission, KIC 8462852 was observed to undergo irregularly
shaped, aperiodic dips in flux of up to∼ 20 per cent. The dipping activity can last for …
shaped, aperiodic dips in flux of up to∼ 20 per cent. The dipping activity can last for …
[HTML][HTML] The JWST Early-release Science Program for Direct Observations of Exoplanetary Systems II: a 1 to 20 μm spectrum of the planetary-mass companion VHS …
We present the highest fidelity spectrum to date of a planetary-mass object. VHS 1256 b is
a< 20 M Jup widely separated (∼ 8'', a= 150 au), young, planetary-mass companion that …
a< 20 M Jup widely separated (∼ 8'', a= 150 au), young, planetary-mass companion that …
Does the use of laminar flow and space suits reduce early deep infection after total hip and knee replacement?: the ten-year results of the New Zealand Joint Registry
GJ Hooper, AG Rothwell, C Frampton… - The Journal of Bone & …, 2011 - boneandjoint.org.uk
We have investigated whether the use of laminar-flow theatres and space suits reduced the
rate of revision for early deep infection after total hip (THR) and knee (TKR) replacement by …
rate of revision for early deep infection after total hip (THR) and knee (TKR) replacement by …
Steady state evolution of debris disks around a stars
This paper confronts a simple analytical model for the steady state evolution of debris disks
due to collisions with Spitzer observations of dust around main-sequence A stars. It is …
due to collisions with Spitzer observations of dust around main-sequence A stars. It is …
Resonant trapping of planetesimals by planet migration: debris disk clumps and Vega's similarity to the Solar System
MC Wyatt - The Astrophysical Journal, 2003 - iopscience.iop.org
This paper describes a model that can explain the observed clumpy structures of debris
disks. Clumps arise because after a planetary system forms, its planets migrate because of …
disks. Clumps arise because after a planetary system forms, its planets migrate because of …