All Stories

  1. From Dust to Nanodust: Resolving Circumstellar Dust from the Colliding-wind Binary Wolf-Rayet 140
  2. Nano-diamonds in proto-planetary discs
  3. Spinning nano-carbon grains: Viable origin for anomalous microwave emission
  4. A derivation of nano-diamond optical constants
  5. Edging towards an understanding of CH/CH2 on nano-diamonds
  6. First MATISSE L-band observations of HD 179218
  7. BEDE: Bayesian estimates of dust evolution for nearby galaxies
  8. Influence of the nano-grain depletion in photon-dominated regions
  9. Spatial distribution of the aromatic and aliphatic carbonaceous nanograin features in the protoplanetary disk around HD 100546
  10. A nearby galaxy perspective on dust evolution
  11. Dust evolution across the Horsehead nebula
  12. JINGLE – IV. Dust, H i gas, and metal scaling laws in the local Universe
  13. High-resolution, 3D radiative transfer modelling
  14. The ISM scaling relations in DustPedia late-type galaxies: A benchmark study for the Local Universe
  15. Dust emissivity and absorption cross section in DustPedia late-type galaxies
  16. From grains to pebbles: the influence of size distribution and chemical composition on dust emission properties
  17. The first maps of κd – the dust mass absorption coefficient – in nearby galaxies, with DustPedia
  18. The essential elements of dust evolution
  19. DustPedia: the relationships between stars, gas, and dust for galaxies residing in different environments
  20. Old and young stellar populations in DustPedia galaxies and their role in dust heating
  21. Carbonaceous nano-dust emission in proto-planetary discs: the aliphatic-aromatic components
  22. A systematic metallicity study of DustPedia galaxies reveals evolution in the dust-to-metal ratios,
  23. Dust emission profiles of DustPedia galaxies
  24. Fraction of bolometric luminosity absorbed by dust in DustPedia galaxies
  25. The Interstellar Dust Properties of Nearby Galaxies
  26. The optical properties of dust: the effects of composition, size, and structure
  27. DustPedia: Multiwavelength photometry and imagery of 875 nearby galaxies in 42 ultraviolet-microwave bands
  28. Dust models compatible with Planck intensity and polarization data in translucent lines of sight
  29. Radial distribution of dust, stars, gas, and star-formation rate in DustPedia face-on galaxies
  30. Interplay of dust alignment, grain growth, and magnetic fields in polarization: lessons from the emission-to-extinction ratio
  31. Modeling dust emission in the Magellanic Clouds with Spitzer and Herschel
  32. DustPedia: A Definitive Study of Cosmic Dust in the Local Universe
  33. The global dust modelling framework THEMIS
  34. The Herschel Virgo Cluster Survey
  35. Dust evolution, a global view I. Nanoparticles, nascence, nitrogen and natural selection … joining the dots
  36. Dust evolution, a global view: II. Top-down branching, nanoparticle fragmentation and the mystery of the diffuse interstellar band carriers
  37. Dust evolution, a global view: III. Core/mantle grains, organic nano-globules, comets and surface chemistry
  38. Dust variations in the diffuse interstellar medium: constraints on Milky Way dust fromPlanck-HFI observations(Corrigendum)
  39. Mantle formation, coagulation, and the origin of cloud/core shine
  40. Mantle formation, coagulation, and the origin of cloud/core shine
  41. H2formation via the UV photo-processing of a-C:H nano-particles
  42. Dust models post-Planck: constraining the far-infrared opacity of dust in the diffuse interstellar medium
  43. Interstellar dust modelling: Interfacing laboratory, theoretical and observational studies (The THEMIS model)
  44. Dust evolution in the transition towards the denser ISM: impact on dust temperature, opacity, and spectral index
  45. Dust variations in the diffuse interstellar medium: constraints on Milky Way dust fromPlanck-HFI observations
  46. DESTRUCTION OF INTERSTELLAR DUST IN EVOLVING SUPERNOVA REMNANT SHOCK WAVES
  47. High-resolution, 3D radiative transfer modeling
  48. A framework for resolving the origin, nature and evolution of the diffuse interstellar band carriers?
  49. A re-evaluation of dust processing in supernova shock waves
  50. Challenges in modelling the reaction chemistry of interstellar dust
  51. Planck intermediate results
  52. A hidden reservoir of Fe/FeS in interstellar silicates?
  53. Gas-to-dust mass ratios in local galaxies over a 2 dex metallicity range
  54. The cycling of carbon into and out of dust
  55. The evolution of amorphous hydrocarbons in the ISM: dust modelling from a new vantage point
  56. The Herschel Virgo Cluster Survey – XIV. Transition-type dwarf galaxies in the Virgo cluster
  57. Dust heating
  58. Heteroatom-doped hydrogenated amorphous carbons, a-C:H:X
  59. The Stability of Cosmic Fullerenes and Fullerenic Aggregates
  60. Dust coagulation processes as constrained by far-infrared observations
  61. THE FORMATION OF COSMIC FULLERENES FROM AROPHATIC CLUSTERS
  62. ON THE EXCITATION AND FORMATION OF CIRCUMSTELLAR FULLERENES
  63. Variations on a theme – the evolution of hydrocarbon solids (Corrigendum)
  64. Variations on a theme – the evolution of hydrocarbon solids (Corrigendum)
  65. Small hydrocarbon particle erosion in a hot gas
  66. Amorphous Hydrocarbon Optical Properties
  67. Variations on a theme – the evolution of hydrocarbon solids
  68. Variations on a theme – the evolution of hydrocarbon solids
  69. Variations on a theme – the evolution of hydrocarbon solids
  70. Planckearly results. XXIV. Dust in the diffuse interstellar medium and the Galactic halo
  71. Planckearly results. XXV. Thermal dust in nearby molecular clouds
  72. Dust Content of Virgo Star-Forming Dwarf Galaxies
  73. Dust in Cluster Dwarf Elliptical Galaxies
  74. Organic materials in planetary and protoplanetary systems: nature or nurture?
  75. Hydroxyl radical production and storage in analogues of amorphous interstellar silicates: a possible “wet” accretion phase for inner telluric planets
  76. Dust destruction in the ISM: a re-evaluation of dust lifetimes
  77. Aggregate dust connections and emissivity enhancements
  78. The characterisation of irregularly-shaped particles
  79. Shocks in dense clouds
  80. Polycyclic aromatic hydrocarbon processing by cosmic rays
  81. The global dust SED: tracing the nature and evolution of dust with DustEM
  82. Herschel/HIFI: first science highlights
  83. The far-infrared view of M87 as seen by the Herschel Space Observatory
  84. FIR colours and SEDs of nearby galaxies observed withHerschel
  85. Herschelspecial feature
  86. TheHerschelVirgo Cluster Survey
  87. TheHerschelVirgo Cluster Survey
  88. TheHerschelVirgo Cluster Survey
  89. TheHerschelVirgo Cluster Survey
  90. TheHerschelVirgo Cluster Survey
  91. TheHerschelVirgo Cluster Survey
  92. TheHerschelVirgo Cluster Survey
  93. Polycyclic aromatic hydrocarbon processing in a hot gas
  94. Polycyclic aromatic hydrocarbon processing in interstellar shocks
  95. Insight from the unexpected
  96. DISTRIBUTION AND CHARACTERISTICS OF INFRARED DARK CLOUDS USING GENETIC FORWARD MODELLING
  97. Dust and the art of Galactic map making
  98. Microwave emission from dust revisited
  99. Interstellar radiation and dust
  100. Shocks in dense clouds
  101. A View of Our Current Knowledge of Dust: Where Do We Go from Here?
  102. Dust dynamics and processing in shocks
  103. Foreword
  104. The evolution of dust in extreme astrophysical environments
  105. The role of dust in the interstellar medium: dust sources and dust evolution
  106. Carbonaceous dust in interstellar shock waves: hydrogenated amorphous carbon (a-C:H) vs. graphite
  107. The 6.2 $\sf \mu{\rm m}$ band position in laboratory and astrophysical spectra: a tracer of the aliphatic to aromatic evolution of interstellar carbonaceous dust
  108. Variations of the Mid‐IR Aromatic Features inside and among Galaxies
  109. The space infrared telescope for cosmology and astrophysics: SPICA A joint mission between JAXA and ESA
  110. Chemical and morphological evolution of a silicate surface under low-energy ion irradiation
  111. The mineralogy of cosmic dust: astromineralogy
  112. Shocks in dense clouds
  113. The Evolution of Dust in the Early Universe with Applications to the Galaxy SDSS J1148+5251
  114. Ferromagnetic inclusions in silicate thin films: insights into the magnetic properties of cosmic grains
  115. IRAS 08572+3915: constraining the aromatic versus aliphatic content of interstellar HACs
  116. The origin of GEMS in IDPs as deduced from microstructural evolution of amorphous silicates with annealing
  117. ISM properties in low-metallicity environments
  118. First determination of the (re)crystallization activation energy of an irradiated olivine-type silicate
  119. ISM properties in low-metallicity environments
  120. Shock Processing of Large Grains in the Interstellar Medium
  121. IR spectroscopic study of olivine, enstatite and diopside irradiated with low energy H$\mathsf{^+}$ and He$\mathsf{^+}$ ions
  122. Surface C–H stretching features on meteoritic nanodiamonds
  123. ISM properties in low-metallicity environments
  124. The role of laboratory experiments in the characterisation of silicon-based cosmic material
  125. Evolution of dust properties in an interstellar filament
  126. Low-energy helium ion irradiation-induced amorphization and chemical changes in olivine: Insights for silicate dust evolution in the interstellar medium
  127. Low-temperature crystallization of MgSiO3glasses under electron irradiation: Possible implications for silicate dust evolution in circumstellar environments
  128. Evolution of very small particles in the southern part of Orion B observed by ISOCAM
  129. Evolution of interstellar dust properties from diffuse medium to a dense cloud
  130. Grain-Grain Coagulation in the ISM
  131. Temperature-dependent FIR/sub-mm dust emissivity indices: some implications for the diffuse ISM dust composition
  132. The Nature of the Low-Metallicity ISM in the Dwarf Galaxy NGC 1569
  133. The evolution of very small dust particles in molecular clouds observed with ISOCAM
  134. Interstellar and circumstellar grain formation and survival
  135. Structural and chemical alteration of crystalline olivine under low energy He+ irradiation
  136. Depletion patterns and dust evolution in the interstellar medium
  137. Dust in the Local Interstellar Wind
  138. Infrared Imaging and Spectroscopy of the Helix with ISOCAM
  139. Infrared spectroscopy of interstellar nanodiamonds from the Orgueil meteorite
  140. The propagation and survival of interstellar grains
  141. Grain Shattering in Shocks: The Interstellar Grain Size Distribution
  142. The Dust Size Distribution and Grain Shattering in Shock Waves
  143. Disintegration of dust aggregates in interstellar shocks and the lifetime of dust grains in the ISM
  144. Disintegration of Dust Aggregates in Interstellar Shocks and the Lifetime of Dust Grains in the ISM
  145. Grain destruction in shocks in the interstellar medium
  146. Infrared emission from hydrogenated amorphous carbon and amorphous carbon grains in the interstellar medium
  147. Simple linear polycyclic aromatic hydrocarbon molecules and the infrared emission features - Mothballs in the Orion ridge?
  148. HAC-coated silicate grains and PAHs in diffuse clouds and low-velocity shocks
  149. Mantle desorption from amorphous grains
  150. Hydrogenated amorphous carbon-coated silicate particles as a source of interstellar extinction
  151. Modelling interstellar extinction - I. Porous grains
  152. Hydrogenated Amorphous Carbon-Coated Silicate Particles: Diamond and Graphite-Like Carbons and Interstellar Extinction
  153. Interstellar extinction correlations
  154. Interplanetary material as a guide to the composition of interstellar grains
  155. Electric charge on ionic grains
  156. Time-dependent sticking coefficients and mantle growth on interstellar grains
  157. The 3  m ice band in Taurus: implications for interstellar chemistry
  158. Chemical effects of irregular interstellar oxide grains
  159. Dust in the Interstellar Medium
  160. Dust composition in the low density medium around spica
  161. Chemical evolution in local interstellar molecular clouds