Search Results - "Greaves, S. J"
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Analysis of the Herschel DEBRIS Sun-like star sample
Published in Monthly notices of the Royal Astronomical Society (11-04-2018)“…Abstract This paper presents a study of circumstellar debris around Sun-like stars using data from the Herschel DEBRIS Key Programme. DEBRIS is an unbiased…”
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Steady State Evolution of Debris Disks around A Stars
Published in The Astrophysical journal (01-07-2007)“…This paper confronts a simple analytical model for the steady state evolution of debris disks due to collisions with Spitzer observations of dust around…”
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99 Herculis: host to a circumbinary polar-ring debris disc
Published in Monthly notices of the Royal Astronomical Society (01-04-2012)“…We present resolved Herschel images of a circumbinary debris disc in the 99 Herculis system. The primary is a late F-type star. The binary orbit is well…”
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Have protoplanetary discs formed planets?
Published in Monthly notices of the Royal Astronomical Society (21-09-2010)“…It has recently been noted that many discs around T Tauri stars appear to comprise only a few Jupiter masses of gas and dust. Using millimetre surveys of discs…”
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Coplanar circumbinary debris discs
Published in Monthly notices of the Royal Astronomical Society (01-11-2012)“…Abstract We present resolved Herschel images of circumbinary debris discs in the α CrB (HD 139006) and β Tri (HD13161) systems. By modelling their structure,…”
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CO emission from discs around isolated HAeBe and Vega-excess stars
Published in Monthly notices of the Royal Astronomical Society (11-05-2005)“…We describe results from a survey for J = 3–2 12CO emission from visible stars classified as having an infrared excess. The line is clearly detected in 21…”
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ALMA and Herschel observations of the prototype dusty and polluted white dwarf G29-38
Published in Monthly notices of the Royal Astronomical Society (21-10-2014)“…ALMA Cycle 0 and Herschel 1 PACS observations are reported for the prototype, nearest, and brightest example of a dusty and polluted white dwarf, G29-38. These…”
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New Debris Disks around Nearby Main-Sequence Stars: Impact on the Direct Detection of Planets
Published in The Astrophysical journal (01-12-2006)“…Using the MIPS instrument on Spitzer, we have searched for infrared excesses around a sample of 82 stars, mostly F, G, and K main-sequence field stars, along…”
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Magnetic fields in planetary nebulae and post-AGB nebulae
Published in Monthly notices of the Royal Astronomical Society (21-03-2007)“…Magnetic fields are an important but largely unknown ingredient of planetary nebulae. They have been detected in oxygen-rich asymptotic giant branch (AGB) and…”
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Debris discs and comet populations around Sun-like stars: the Solar system in context
Published in Monthly notices of the Royal Astronomical Society (01-06-2010)“…Numerous nearby FGK dwarfs possess discs of debris generated by collisions among comets. Here, we fit the levels of dusty excess observed by Spitzer at 70 μm…”
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Steady-state evolution of debris discs around solar-type stars
Published in Monthly notices of the Royal Astronomical Society (01-07-2011)“…We present an analysis of debris disc data around Solar-type stars (spectral types F0-K5) using the steady-state analytical model of Wyatt et al. Models are…”
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The JCMT Legacy Survey of the Gould Belt: mapping 13CO and C18O in Orion A
Published in Monthly notices of the Royal Astronomical Society (01-05-2012)“…The Gould Belt Legacy Survey will map star-forming regions within 500 pc, using Heterodyne Array Receiver Programme (HARP), Submillimetre Common-User Bolometer…”
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Target selection for the SUNS and DEBRIS surveys for debris discs in the solar neighbourhood
Published in Monthly notices of the Royal Astronomical Society (11-04-2010)“…Debris discs – analogous to the asteroid and Kuiper–Edgeworth belts in the Solar system – have so far mostly been identified and studied in thermal emission…”
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Discovery of carbon monoxide in the upper atmosphere of Pluto
Published in Monthly notices of the Royal Astronomical Society. Letters (11-06-2011)“…ABSTRACT Pluto’s icy surface has changed colour and its atmosphere has swelled since its last closest approach to the Sun in 1989. The thin atmosphere is…”
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Synthesis of Hydrophilic Polymer-Grafted Ultrafine Inorganic Oxide Particles in Protic Media at Ambient Temperature via Atom Transfer Radical Polymerization: Use of an Electrostatically Adsorbed Polyelectrolytic Macroinitiator
Published in Langmuir (03-02-2004)“…A new approach for the surface grafting of polymer chains to colloidal substrates is described. A cationic macroinitiator has been designed for the surface…”
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Synthesis of Vinyl Polymer−Silica Colloidal Nanocomposites Prepared Using Commercial Alcoholic Silica Sols
Published in Langmuir (16-03-2004)“…The surfactant-free synthesis of vinyl polymer−silica nanocomposite particles has been achieved in aqueous alcoholic media at ambient temperature in the…”
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Origin of the metallicity dependence of exoplanet host stars in the protoplanetary disc mass distribution
Published in Monthly notices of the Royal Astronomical Society (01-10-2007)“…The probability of a star hosting a planet that is detectable in radial velocity surveys increases as Ppl(Z) ∝ (10Z)2, where Z is stellar metallicity. Models…”
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The JCMT Legacy Survey of the Gould Belt: a first look at Serpens with HARP
Published in Monthly notices of the Royal Astronomical Society (21-12-2010)“…The Gould Belt Legacy Survey on the James Clerk Maxwell Telescope's has observed a region of 260 arcmin2 in 12CO J= 3 → 2 emission, and a 190 arcmin2 subset of…”
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Synthesis of Vinyl Polymer−Silica Colloidal Nanocomposites via Aqueous Dispersion Polymerization
Published in Langmuir (18-03-2003)“…The surfactant-free synthesis of colloidal dispersions of vinyl polymer−silica nanocomposite particles in aqueous media using a batch emulsion polymerization…”
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Submillimeter Images of a Dusty Kuiper Belt around η Corvi
Published in The Astrophysical journal (10-02-2005)“…We present submillimeter and mid-IR images of the circumstellar disk around the nearby F2 V star eta Corvi. The disk is resolved at 850 mu m with a size of…”
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