Search Results - "DENT, W. R. F"
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DUST AND GAS IN THE DISK OF HL TAURI: SURFACE DENSITY, DUST SETTLING, AND DUST-TO-GAS RATIO
Published in The Astrophysical journal (01-01-2016)“…ABSTRACT The recent ALMA observations of the disk surrounding HL Tau reveal a very complex dust spatial distribution. We present a radiative transfer model…”
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A Highly Settled Disk around Oph163131
Published in The Astrophysical journal (01-05-2022)“…Abstract High dust density in the midplane of protoplanetary disks is favorable for efficient grain growth and can allow fast formation of planetesimals and…”
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Submillimetre dust polarization and opacity in the HD163296 protoplanetary ring system
Published in Monthly notices of the Royal Astronomical Society. Letters (01-01-2019)“…ABSTRACT We present ALMA images of the sub-mm continuum polarization and spectral index of the protoplanetary ringed disc HD163296. The polarization fraction…”
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Exocometary Gas in the HD 181327 Debris Ring
Published in Monthly notices of the Royal Astronomical Society (11-08-2016)“…An increasing number of observations have shown that gaseous debris discs are not an exception. However, until now, we only knew of cases around A stars. Here…”
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Detection of Rydberg Lines from the Atmosphere of Betelgeuse
Published in Astrophysical journal. Letters (01-05-2024)“…Abstract Emission lines from Rydberg transitions are detected for the first time from a region close to the surface of Betelgeuse. The H30 α line is observed…”
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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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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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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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HERSCHEL PACS OBSERVATIONS AND MODELING OF DEBRIS DISKS IN THE TUCANA-HOROLOGIUM ASSOCIATION
Published in The Astrophysical journal (10-07-2012)“…We present Herschel PACS photometry of 17 B- to M-type stars in the 30 Myr old Tucana-Horologium Association. This work is part of the Herschel Open Time Key…”
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A large-scale CO survey of the Rosette Molecular Cloud: assessing the effects of O stars on surrounding molecular gas
Published in Monthly notices of the Royal Astronomical Society (01-06-2009)“…We present a new large-scale survey of the J= 3–2 12CO emission covering 4.8 deg2 around the Rosette Nebula. The results reveal the complex dynamics of the…”
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Nine Localized Deviations from Keplerian Rotation in the DSHARP Circumstellar Disks: Kinematic Evidence for Protoplanets Carving the Gaps
Published 10-02-2020“…We present evidence for localized deviations from Keplerian rotation, I.e., velocity "kinks," in 8 of the 18 circumstellar disks observed by the DSHARP…”
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Has the dust clump in the debris disc of Beta Pictoris moved?
Published in Monthly notices of the Royal Astronomical Society (09-01-2023)“…ABSTRACT The edge-on debris disc of the nearby young star Beta Pictoris shows an unusual brightness asymmetry in the form of a clump. The clump has been…”
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Molecular Reconnaissance of the β Pictoris Gas Disk with the SMA: A Low HCN/(CO+CO2) Outgassing Ratio and Predictions for Future Surveys
Published in The Astrophysical journal (01-02-2018)“…The exocometary origin of CO gas has been confirmed in several extrasolar Kuiper belts, with CO ice abundances consistent with solar system comets. We here…”
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Molecular Gas Clumps from the Destruction of Icy Bodies in the β Pictoris Debris Disk
Published in Science (American Association for the Advancement of Science) (28-03-2014)“…Many stars are surrounded by disks of dusty debris formed in the collisions of asteroids, comets, and dwarf planets, but is gas also released in such events?…”
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Gas and dust around A-type stars at tens of Myr: signatures of cometary breakup
Published in Monthly notices of the Royal Astronomical Society (01-10-2016)“…Discs of dusty debris around main-sequence stars indicate fragmentation of orbiting planetesimals, and for a few A-type stars, a gas component is also seen…”
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The circumstellar disc around the Herbig AeBe star HD169142
Published in Monthly notices of the Royal Astronomical Society (01-02-2006)“…We present 7 mm and 3.5 cm wavelength continuum observations towards the Herbig AeBe star HD169142 performed with the Very Large Array (VLA) with an angular…”
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CO mass upper limits in the Fomalhaut ring – the importance of NLTE excitation in debris discs and future prospects with ALMA
Published in Monthly notices of the Royal Astronomical Society (11-03-2015)“…In recent years, gas has been observed in an increasing number of debris discs, though its nature remains to be determined. Here, we analyse CO molecular…”
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ALMA observations of the η Corvi debris disc: inward scattering of CO-rich exocomets by a chain of 3–30 M ⊕ planets?
Published in Monthly notices of the Royal Astronomical Society (01-03-2017)“…While most of the known debris discs present cold dust at tens of astronomical unit (au), a few young systems exhibit hot dust analogous to the Zodiacal dust…”
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Exocometary gas structure, origin and physical properties around β Pictoris through ALMA CO multitransition observations
Published in Monthly notices of the Royal Astronomical Society (01-01-2017)“…Recent ALMA observations unveiled the structure of CO gas in the 23 Myr old beta Pictoris planetary system, a component that has been discovered in many…”
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LMT/AzTEC observations of Vega
Published in Monthly notices of the Royal Astronomical Society (28-06-2022)“…ABSTRACT Vega is the prototypical debris disc system. Its architecture has been extensively studied at optical to millimetre wavelengths, revealing a near…”
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