Evolution of Debris Disks

By M. C. Wyatt. 2008

746 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/72dca707102354d7cb5164437986524c610c6554

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In Astronomy and Astrophysics

Citations in the corpus

Protoplanetary disk lifetimes vs stellar mass and possible implications for giant planet populations (2015, background): “However, the evolution of disks is thought to remove dust from the inner regions (e.g. Koepferl et al. 2013; Alexander et al. 2014, R14), leaving only mid-IR (24 µm) or even far-IR (>50 µm) excesses as in the case of transitional and debris disks (Wyatt 2008; Williams & Cieza 2011).”
Imaging Extrasolar Giant Planets (2016, background): “Topical reviews by Zuckerman (2001), Moro-Martin et al. (2008), Wyatt (2008), Krivov (2010), and Matthews et al. (2014a) high- 7 light recent theoretical and observational progress on the formation, modeling, and evolution of debris disks.”
The Ages of Stars (2007, background): “Evans et al. (2009) present a comprehensive look at the formation phases in nearby star-forming regions and estimate relative timescales and durations, and Wyatt (2008) reviews the evolution of debris disks.”
THE VECTOR VORTEX CORONAGRAPH: LABORATORY RESULTS AND FIRST LIGHT AT PALOMAR OBSERVATORY (2009, background): “However, the few exoplanets and the majority of circumstellar disks imaged so far all required high contrast (Absil & Mawet 2010; Oppenheimer & Hinkley 2009; Duchêne 2008; Wyatt 2008).”
Protoplanetary disc evolution and dispersal: the implications of X-ray photoevaporation (2010, methodology): “Figure 15 shows a plot of the fractional excess of the disc compared with the stellar photosphere at 24µm and 70µm, where we compare our models with observations of objects classified as young debris discs around solar-type stars (Wyatt 2008).”
ALMA SURVEY OF LUPUS PROTOPLANETARY DISKS. I. DUST AND GAS MASSES (2016, methodology): “We measured a mean signal of 0.08 ± 0.06 mJy, which gives a 3σ upper limit on the average dust mass of individually undetected continuum sources of ∼6 Lunar masses (0.03 M⊕), comparable to debris disk levels (Wyatt 2008).”
SCUBA-2: the 10 000 pixel bolometer camera on the James Clerk Maxwell Telescope (2013, background): “…1998), pin-pointing cold dense regions in molecular clouds where new stars are forming (e.g. Motte et al. 1998; André et al. 2010), and imaging of vast clouds of cold dust around nearby stars believed to be analogues of the Kuiper Belt in our Solar System (e.g. Holland et al. 1998; Wyatt 2008).”
Improved angular momentum evolution model for solar-like stars (2013, background): “…accretion measurements indicate that nearly all stars are born with a disk, that the disk fraction decreases to about 50% by an age of 3 Myr, and only a small proportion of stars are still surrounded by a disk at an age of 10 Myr (e.g., Hernández et al. 2008; Wyatt 2008; Williams & Cieza 2011).”
Adaptive Optics for Astronomy (2012, background): “Many circumstellar debris disks do show significant sub-structure, which is believed to be driven by orbiting companions, and can provide insights into the mechanisms of planet formation (Wyatt 2008).”
Dynamics of Protoplanetary Disks (2010, background): “A clear demarcation does separate protoplanetary disks from debris disks; dusty gas-poor structures around older stars whose properties reflect the collisional evolution of a population of small bodies (Wyatt 2008).”
NEW DEBRIS DISKS AROUND YOUNG, LOW-MASS STARS DISCOVERED WITH THE SPITZER SPACE TELESCOPE (2009, neutral): “The collisions of parent bodies decay with time (e.g., Wyatt 2008; Kenyon & Bromley 2005, and references therein).”
An ALMA Survey of Protoplanetary Disks in the σ Orionis Cluster (2017, background): “6 Lunar masses (0.03 M⊕), comparable to debris disk levels (Wyatt 2008).”
Our astrochemical heritage (2012, background): “Debris disks are also observed, with their poor gas content and with evidence of large grains and/or planets ([475];”
TOWARD A DETERMINISTIC MODEL OF PLANETARY FORMATION. VI. DYNAMICAL INTERACTION AND COAGULATION OF MULTIPLE ROCKY EMBRYOS AND SUPER-EARTH SYSTEMS AROUND SOLAR-TYPE STARS (2010, background): “Debris from such collisions would produce “cold” grains that reprocess stellar radiation and generate far-infrared excess radiation (Wyatt 2008).”
Protoplanetary Disks and Their Evolution (2011, background): “There are also several related reviews that have been recently written for this series including the inner disk (Dullemond & Monnier 2010), debris disks (Wyatt 2008), and dynamical processes (Armitage 2010).”
Debris disks as signposts of terrestrial planet formation (2011, methodology): “The reader is referred to other work discussing current dust detection limits at short (Absil et al. 2006; Akeson et al. 2009) and long (Smith et al. 2009) wavelengths (see also Wyatt 2008).”
YOUNG STELLAR OBJECTS IN THE GOULD BELT (2015, background): “• Adopting standard assumptions, we derive durations of 0.40 − 0.78 Myr for Class 0+I YSOs and 0.26−0.50 Myr for Flat-spectrum YSOs, with most likely durations of 0.46−0.72 Myr (Class 0+I) and 0.30 − 0.46 Myr (Flat-spectrum).”