All Stories

  1. Experimental investigation of O 2 diffusion and entrapment in interstellar amorphous solid water
  2. In situ characterization of volatile and refractory hydrocarbons produced by UV photolysis of interstellar C 2 H 2 ice
  3. Laboratory Infrared Spectra and Band Strengths of Carbonyl Sulfide (OCS) in CH3OH- and CO-Rich Ice Mixtures for Analyzing Interstellar Ice Observations
  4. Ozone in Planetary Ices: Solid-State Detection under Enceladus-like conditions
  5. Ammonium hydrosulfide (NH4SH) as a potentially significant sulfur sink in interstellar ices
  6. Production of linear alkanes via the solid-state hydrogenation of interstellar polyynes
  7. Formation of carbonyl sulfide (OCS) via SH radicals in interstellar CO-rich ice under dense cloud conditions
  8. Formation of S-Bearing Complex Organic Molecules in Interstellar Clouds via Ice Reactions with C2H2, HS, and Atomic H
  9. Formation of N–bearing complex organic molecules in molecular clouds: Ketenimine, acetonitrile, acetaldimine, and vinylamine via the UV photolysis of C2H2 ice
  10. A deep search for large complex organic species toward IRAS16293-2422 B at 3 mm with ALMA
  11. Pulsed ion deflection to overcome detector saturation in cryogenic ice sampling
  12. Spatially resolving the volatile sulfur abundance in the HD 100546 protoplanetary disk
  13. Interstellar Carbonaceous Dust Erosion Induced by X-Ray Irradiation of Water Ice in Star-forming Regions
  14. Interaction of H2S with H atoms on grain surfaces under molecular cloud conditions
  15. The hunt for formamide in interstellar ices
  16. Resonant infrared irradiation of CO and CH3OH interstellar ices
  17. Condensation of Atomic Carbon: Routes Towards Organics
  18. Formation of Complex Molecules in the Translucent Phase via “non-energetic” Processing on C$$_\textbf{2}$$H$$_\textbf{2}$$ Ice
  19. ­Laboratory studies of irradiated Enceladus ice analogues
  20. Formation of the Simplest Amide in Molecular Clouds: Formamide (NH2CHO) and Its Derivatives in H2O-rich and CO-rich Interstellar Ice Analogs upon VUV Irradiation
  21. First Experimental Confirmation of the CH3O + H2CO → CH3OH + HCO Reaction: Expanding the CH3OH Formation Mechanism in Interstellar Ices
  22. Methoxymethanol formation starting from CO hydrogenation
  23. Methane Formation in Cold Regions from Carbon Atoms and Molecular Hydrogen
  24. A pathway to peptides in space through the condensation of atomic carbon
  25. Hydrogenation of Accreting C Atoms and CO Molecules–Simulating Ketene and Acetaldehyde Formation Under Dark and Translucent Cloud Conditions
  26. Quantification of O2 formation during UV photolysis of water ice: H2O and H2O:CO2 ices
  27. Formation of complex organic molecules in molecular clouds: acetaldehyde, vinyl alcohol, ketene, and ethanol via the “energetic” processing of C2H2 ice
  28. A non-energetic mechanism for glycine formation in the interstellar medium
  29. A cryogenic ice setup to simulate carbon atom reactions in interstellar ices
  30. An experimental study of the surface formation of methane in interstellar molecular clouds
  31. Formation of complex molecules in translucent clouds: acetaldehyde, vinyl alcohol, ketene, and ethanol via “nonenergetic” processing of C2H2 ice
  32. Searches for Interstellar HCCSH and H2CCS
  33. Formation of interstellar propanal and 1-propanol ice: a pathway involving solid-state CO hydrogenation
  34. Extension of the HCOOH and CO2 solid-state reaction network during the CO freeze-out stage: inclusion of H2CO
  35. Alcohols on the Rocks: Solid-State Formation in a H3CC≡CH + OH Cocktail under Dark Cloud Conditions
  36. H2 photochemistry in interstellar ices:The formation of HCO in UV irradiated CO:H2 ice mixtures
  37. Synthesis of solid-state complex organic molecules through accretion of simple species at low temperatures
  38. H2 chemistry in interstellar ices: the case of CO ice hydrogenation in UV irradiated CO:H2 ice mixtures
  39. Formation of interstellar methanol ice prior to the heavy CO freeze-out stage
  40. Reactive Desorption of CO Hydrogenation Products under Cold Pre-stellar Core Conditions
  41. Formation of Glycerol through Hydrogenation of CO Ice under Prestellar Core Conditions
  42. Solid-state production of complex organic molecules: H-atom addition versus UV irradiation
  43. Production of complex organic molecules:H-atom addition versus UV irradiation
  44. Simultaneous hydrogenation and UV-photolysis experiments of NO in CO-rich interstellar ice analogues; linking HNCO, OCN−, NH2CHO, and NH2OH
  45. CHEMICAL EVOLUTION OF A CO ICE INDUCED BY SOFT X-RAYS
  46. Controlling the emission profile of an H2discharge lamp to simulate interstellar radiation fields
  47. H-atom addition and abstraction reactions in mixed CO, H2CO and CH3OH ices – an extended view on complex organic molecule formation
  48. FORMATION OF S-BEARING SPECIES BY VUV/EUV IRRADIATION OF H2S-CONTAINING ICE MIXTURES: PHOTON ENERGY AND CARBON SOURCE EFFECTS
  49. Relevance of the H2 + O reaction pathway for the surface formation of interstellar water
  50. VACUUM ULTRAVIOLET EMISSION SPECTRUM MEASUREMENT OF A MICROWAVE-DISCHARGE HYDROGEN-FLOW LAMP IN SEVERAL CONFIGURATIONS: APPLICATION TO PHOTODESORPTION OF CO ICE
  51. SOFT X-RAY IRRADIATION OF METHANOL ICE: FORMATION OF PRODUCTS AS A FUNCTION OF PHOTON ENERGY