About: Antony Jones

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About: Antony Jones Goto Sponge NotDistinct Permalink

An Entity of Type : foaf:Person, within Data Space : data.idref.fr associated with source document(s)

Attributes	Values
type	Person
sameAs	Jones, Antony Jones, Antony Jones, Antony Jones, Antony Jones, Antony
bnf-onto:FRBNF	13770492(xsd:integer)
preferred label	Jones, Antony
name	Antony Jones
Language	http://lexvo.org/id/iso639-3/eng
isni:identifierValid	0000000081222545
Given name	Antony
familyName	Jones
note	En poste : Centre d'études spatiales des rayonnements, Toulouse, (en 1999)
gender	male
ORCID iD	0000-0003-0577-6425
is sameAs of	Jones, Antony
is Author of	Dust coagulation processes as constrained by far-infrared observations The Herschel Virgo Cluster Survey The role of dust in the interstellar medium: dust sources and dust evolution The nature of coagulated interstellar grains as contrained by FIR and sub-mm observations Herschel/HIFI: first science highlights Variations on a theme - the evolution of hydrocarbon solids ( Corrigendum) DustPedia: Multiwavelength photometry and imagery of 875 nearby galaxies in 42 ultraviolet-microwave bands The essential elements of dust evolution Dust coagulation processes as constrained by far-infrared observations Mantle formation, coagulation, and the origin of cloud/core shine Spatial distribution of the aromatic and aliphatic carbonaceous nanograin features in the protoplanetary disk around HD 100546 Dust emissivity in resolved spiral galaxies A systematic metallicity study of DustPedia galaxies reveals evolution in the dust-to-metal ratios The space infrared telescope for cosmology and astrophysics: SPICA A joint mission between JAXA and ESA Ferromagnetic inclusions in silicate thin films: insights into the magnetic properties of cosmic grains Gas-to-dust mass ratios in local galaxies over a 2 dex metallicity range Surface C-H stretching features on meteoritic nanodiamonds The Herschel Virgo Cluster Survey The Herschel Virgo Cluster Survey Shocks in dense clouds A hidden reservoir of Fe/FeS in interstellar silicates? Dust evolution in the transition towards the denser ISM: impact on dust temperature, opacity, and spectral index Aggregate dust connections and emissivity enhancements Hydroxyl radical production and storage in analogues of amorphous interstellar silicates: a possible “wet” accretion phase for inner telluric planets Dust variations in the diffuse interstellar medium: constraints on Milky Way dust from Planck-HFI observations H 2 formation via the UV photo-processing of a-C:H nano-particles Variations on a theme - the evolution of hydrocarbon solids PDRs4All Influence of the nano-grain depletion in photon-dominated regions From grains to pebbles: the influence of size distribution and chemical composition on dust emission properties Planck intermediate results. XVII. Emission of dust in the diffuse interstellar medium from the far-infrared to microwave frequencies The optical properties of dust: the effects of composition, size, and structure Disintegration of dust aggregates in interstellar shocks and the lifetime of dust grains in the ISM Chemical effects of irregular interstellar oxide grains ISM properties in low-metallicity Environments : III The dust spectral Energy distibution of II Zw 40, He 2-10 and NGC 1140 Dust models compatible with Planck intensity and polarization data in translucent lines of sight The global dust SED: tracing the nature and evolution of dust with DustEM Foreword The Herschel Virgo Cluster Survey Herschel special feature Variations on a theme - the evolution of hydrocarbon solids A re-evaluation of dust processing in supernova shock waves Influence of the nano-grain depletion in photon-dominated regions: Application to the gas physics and chemistry in the Horsehead Gas-to-dust mass ratios in local galaxies over a 2 dex metallicity range Interstellar radiation and dust First MATISSE L-band observations of HD 179218 Heteroatom-doped hydrogenated amorphous carbons, a-C:H: X Mantle formation, coagulation, and the origin of cloud/core shine Small hydrocarbon particle erosion in a hot gas DustPedia: the relationships between stars, gas, and dust for galaxies residing in different environments Polycyclic aromatic hydrocarbon processing in a hot gas Polycyclic aromatic hydrocarbon processing by cosmic rays Planck early results . XXIV . Dust in the diffuse interstellar medium and the Galactic halo The evolution of amorphous hydrocarbons in the ISM: dust modelling from a new vantage point The optical properties of dust: the effects of composition, size, and structure The Herschel Virgo Cluster Survey Microwave emission from dust revisited The global dust SED: tracing the nature and evolution of dust with DustEM A derivation of nano-diamond optical constants The Herschel Virgo Cluster Survey Nano-diamonds in proto-planetary discs Dust models compatible with Planck intensity and polarization data in translucent lines of sight Old and young stellar populations in DustPedia galaxies and their role in dust heating Variations on a theme - the evolution of hydrocarbon solids A nearby galaxy perspective on dust evolution Hydroxyl radical production and storage in analogues of amorphous interstellar silicates: a possible “wet” accretion phase for inner telluric planets Variations on a theme - the evolution of hydrocarbon solids ( Corrigendum) Shocks in dense clouds Dust dynamics and processing in shocks High-resolution, 3D radiative transfer modelling Polycyclic aromatic hydrocarbon processing in interstellar shocks The Herschel Virgo Cluster Survey A View of Our Current Knowledge of Dust: Where Do We Go from Here? Dust destruction in the ISM: a re-evaluation of dust lifetimes Dust models post- Planck: constraining the far-infrared opacity of dust in the diffuse interstellar medium FIR colours and SEDs of nearby galaxies observed with Herschel High-resolution, 3D radiative transfer modeling Dust variations in the diffuse interstellar medium: constraints on Milky Way dust from Planck-HFI observations (Corrigendum) Edging towards an understanding of CH/CH 2 on nano-diamonds Planck early results . XXV . Thermal dust in nearby molecular clouds The evolution of dust in extreme astrophysical environments The characterisation of irregularly-shaped particles Organic materials in planetary and protoplanetary systems: nature or nurture?

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