All Stories

  1. Stellar origin of the 182Hf cosmochronometer and the presolar history of solar system matter
  2. LITHIUM ABUNDANCES IN GLOBULAR CLUSTER GIANTS: NGC 6218 (M12) AND NGC 5904 (M5)
  3. Which physics determines the location of the mean molecular weight minimum in red giants?
  4. Super and massive AGB stars - III. Nucleosynthesis in metal-poor and very metal-poor stars - Z = 0.001 and 0.0001
  5. ON THE NECESSITY OF COMPOSITION-DEPENDENT LOW-TEMPERATURE OPACITY IN MODELS OF METAL-POOR ASYMPTOTIC GIANT BRANCH STARS
  6. The Dawes Review 2: Nucleosynthesis and Stellar Yields of Low- and Intermediate-Mass Single Stars
  7. Super and massive AGB stars - II. Nucleosynthesis and yields - Z = 0.02, 0.008 and 0.004
  8. What asteroseismology can teach us about low-mass core helium burning models
  9. Sodium content as a predictor of the advanced evolution of globular cluster stars
  10. On the internal pollution mechanisms in the globular cluster NGC 6121 (M4): heavy-element abundances and AGB models
  11. CYANOGEN IN NGC 1851 RED GIANT BRANCH AND ASYMPTOTIC GIANT BRANCH STARS: QUADRIMODAL DISTRIBUTIONS
  12. Short‐lived radioactivity in the early solar system: The Super‐AGB star hypothesis
  13. The end of super AGB and massive AGB stars
  14. THE ROLE OF THERMOHALINE MIXING IN INTERMEDIATE- AND LOW-METALLICITY GLOBULAR CLUSTERS
  15. Three-dimensional modelling of proton ingestion episodes in low-mass stars
  16. The evolution and C, N and O yields of intermediate-mass Z = 10[sup −5] stars in isolation and in close binary systems
  17. COMMISSION 35: STELLAR CONSTITUTION
  18. WORKING GROUP on ABUNDANCES IN RED-GIANTS
  19. THREE-DIMENSIONAL HYDRODYNAMICAL SIMULATIONS OF A PROTON INGESTION EPISODE IN A LOW-METALLICITY ASYMPTOTIC GIANT BRANCH STAR
  20. THERMOHALINE MIXING AND ITS ROLE IN THE EVOLUTION OF CARBON AND NITROGEN ABUNDANCES IN GLOBULAR CLUSTER RED GIANTS: THE TEST CASE OF MESSIER 3
  21. COMMISSION 35: STELLAR CONSTITUTION
  22. Lithium production by thermohaline mixing in low-mass, low-metallicity asymptotic giant branch stars
  23. The depletion of carbon by extra mixing in metal-poor giants
  24. Welcoming new players to the stage
  25. O and Na abundance patterns in open clusters of the Galactic disk
  26. A LARGE C+N+O ABUNDANCE SPREAD IN GIANT STARS OF THE GLOBULAR CLUSTER NGC 1851
  27. BLUE STRAGGLERS AFTER THE MAIN SEQUENCE
  28. Why Do Low-Mass Stars Become Red Giants?
  29. montage: AGB Nucleosynthesis with Full s-Process Calculations
  30. The Origin of Elements Heavier than Iron: in Honour of the 70th Birthday of Roberto Gallino
  31. DIVISION IV / WORKING GROUP ABUNDANCES IN RED-GIANTS
  32. Evolution and nucleosynthesis of extremely metal-poor and metal-free low- and intermediate-mass stars
  33. Fluorine in carbon-enhanced metal-poor stars: a binary scenario
  34. Compulsory Deep Mixing of3He and CNO Isotopes in the Envelopes of Low‐Mass Red Giants
  35. A Small Step on the Long Road to Understanding the R Stars: CNO Cycling in Candidate R Star Progenitors
  36. Fifty Years of Nuclear Astrophysics: A Foreword
  37. Structural and Nucleosynthetic Evolution of Metal‐poor & Metal‐free Low and Intermediate Mass Stars
  38. DIVISION IV / WG: ABUNDANCES IN RED GIANTS
  39. Abundances in intermediate-mass AGB stars undergoing third dredge-up and hot-bottom burning
  40. Origin of the early-type R stars: a binary-merger solution to a century-old problem?
  41. Origin of abundance inhomogeneity in globular clusters
  42. Stellar Models and Yields of Asymptotic Giant Branch Stars
  43. Deep Mixing of 3He: Reconciling Big Bang and Stellar Nucleosynthesis
  44. The Chemical Evolution of Helium in Globular Clusters: Implications for the Self‐Pollution Scenario
  45. On the asymptotic giant branch star origin of peculiar spinel grain OC2
  46. Silicon and Carbon Isotopic Ratios in AGB Stars: SiC Grain Data, Models, and the Galactic Evolution of the Si Isotopes
  47. Heavy‐Element Abundances in Giant Stars in 47 Tucanae
  48. Joint Discussion 11 Pre-solar grains as astrophysical tools
  49. The destruction of 3He by Rayleigh-Taylor instability on the first giant branch
  50. Three‐dimensional Numerical Experimentation on the Core Helium Flash of Low‐Mass Red Giants
  51. Nuclear reaction rate uncertainties and astrophysical modeling: Carbon yields from low-mass giants
  52. Abundance Anomalies in Globular Cluster Stars
  53. Working Group on Abundances in Red Giants
  54. Fluorine Abundance Variations in Red Giants of the Globular Cluster M4 and Early‐Cluster Chemical Pollution
  55. Abundance Anomalies in NGC6752 - Do AGB Stars Have a Role?
  56. The Evolution of Fluorine in Galactic Systems
  57. What we do and do not know about the s-process in AGB stars
  58. Reaction Rate Uncertainties and the Production of19F in Asymptotic Giant Branch Stars
  59. On the origin of fluorine in the Milky Way
  60. Modelling self-pollution of globular clusters from asymptotic giant branch stars
  61. Evolution, Nucleosynthesis, and Pulsation of AGB Stars
  62. s‐Process Nucleosynthesis in Asymptotic Giant Branch Stars: A Test for Stellar Evolution
  63. Chemical enrichment by Wolf--Rayet and asymptotic giant branch stars
  64. The Chemical Evolution of Magnesium Isotopic Abundances in the Solar Neighbourhood
  65. Production of Aluminium and the Heavy Magnesium Isotopes in Asymptotic Giant Branch Stars
  66. The Sixth Torino Workshop
  67. AGB Stars and the Observed Abundance of Neon in Planetary Nebulae
  68. AGB stars: summary and warning
  69. Structure, Evolution, and Nucleosynthesis of Primordial Stars
  70. An attempt to model globular cluster red giant abundance anomalies with a simulated hydrogen shell instability
  71. Parameterising the Third Dredge-up in Asymptotic Giant Branch Stars
  72. Galactic Evolution of 7Li: Observational Clues for Models
  73. Galactic Chemical Evolution of Lithium: Interplay between Stellar Sources
  74. Mg and Al abundances in early globular cluster evolution
  75. Eccentricities of the Barium Stars
  76. The eccentricities of the barium stars
  77. Degenerate Thermal Pulses in Asymptotic Giant Branch Stars
  78. Hot bottom burning nucleosynthesis in 6 M⊙ stellar models
  79. Nucleosynthesis of elements in low to intermediate mass stars through the AGB phase
  80. The Asymptotic Giant Branch
  81. On the Numerical Treatment and Dependence of the Third Dredge‐up Phenomenon
  82. Energy generation in convective shells of low-mass, low-metallicity asymptotic giant branch stars
  83. The Third Dredge-Up: Status and Problems
  84. Numerical Modelling of Star Formation in Giant Molecular Clouds
  85. Gravitational fragmentation - A comparison with W49A
  86. A simulation of the collapse and fragmentation of cooling molecular clouds
  87. Stellar evolutionary models from the zero-age main sequence to the first thermal pulse
  88. A Hydrodynamical Model for the Fragmentation of the W49A Star-Forming Region
  89. A Hydrodynamical Study of Fragmenting Gas Clouds
  90. Hydrodynamical Simulations of Collisions between Interstellar Cloudsa
  91. Photofission production of technetium and synthetic asymptotic giant branch evolution
  92. Collisions between high-latitude clouds - Theory meets observations
  93. Starting with stars
  94. Carbon dredge-up in low-mass stars and solar metallicity stars
  95. The formation of a 1.5-solar mass carbon star with Mbol = -4.4
  96. Asymptotic Giant Branch Evolution in the Magellanic Clouds
  97. The asymptotic giant branch evolution of 1.0-3.0 solar mass stars as a function of mass and composition
  98. Controlling Penetration
  99. Interstellar cloud collisions
  100. The effect of grain sedimentation on stellar evolution
  101. Grain Sedimentation and Main Sequence Evolution
  102. Collisions between high latitude clouds: Theory meets observations