Astrochemistry VII (Iau S332): Through the Cosmos from Galaxies to Planets

ISBN-13: 9781107192577 / Angielski / Twarda / 2018 / 462 str.

Maria Cunningham; Tom Millar; Yuri Aikawa

Opis

Reviews how observations of organic molecules in space, numerical models and laboratory studies are used to study the Universe's evolution.

Spis treści

Opening address; 1. Atoms and molecules at high redshifts; 2. Ultra-luminous extragalactic chemistry; 3. Observations of a hot molecular core in a low metallicity dwarf galaxy; 4. The ALMA view of UV-irradiated molecular cloud edges; 5. High-temperature chemistry in external galaxies; 6. Low metallicity ISM: physical properties of the gas and dust; 7. Fire from Ice – massive star birth from infrared dark clouds; 8. Tracing the evolution of massive protostars; 9. Chemical change in the disk forming region of IRAS 16293-2422 studied with ALMA; 10. A molecular outflow-prestellar core interaction in L1689N; 11. The excitation and emission spectrum of the hydrogen molecular ion; 12. The molecular inventory of diffuse clouds; 13. Barnard 1b; 14. Astrochemistry of light hydrides with SOFIA; 15. Theoretical approaches to surface chemistry; 16. Molecule and dust formation in late-type stars; 17. Dust formation at cryogenic temperatures; 18. Simulations of branched carbon-chain chemistry in star-forming regions; 19. The photochemical evolution of the interstellar PAH family; 20. Laboratory astrochemistry; 21. Exploring molecular complexity in the Galactic Center with ALMA; 22. Imaging the water snowline in protostellar envelopes; 23. Chemical tracers of dynamics in low-mass protostellar objects; 24. Protostellar Interferometric Line Survey (PILS); 25. Herschel observations of molecular emission lines in low- and intermediate-mass evolved stars; 26. Interstellar reaction screening via microwave spectral taxonomy; 27. Isotopic fractionation in interstellar molecules; 28. Insights into astrochemistry – highlights from the Rosetta mission; 29. On the origin of O2, N2, and other volatile species in comets; 30. ALMA observations of Titan's atmospheric chemistry and seasonal variation; 31. The chemical connection between 67P/C-G and IRAS16293; 32. Nitrogen fractionation in star-forming regions and primitive Solar System materials; 33. Spatially resolved organic chemistry in protoplanetary disks; 34. Unveiling the mid-plane temperature and mass distribution in the giant-planet formation zone; 35. Zooming in on the physics and chemistry of protoplanetary disks with ALMA; 36. Different dust and gas radial extents in protoplanetary disks; 37. ALMA detection of gas-phase methanol in a planet-forming disk; 38. Measuring gas masses and carbon depletion in young disks; 39. Dust in transition disks; 40. Nitrogen fractionation in protoplanetary disks from the H13CN/HC15N ratio; 41. Models of nitrogen isotope fractionation in protoplanetary disks; 42. Chemistry and evolution of the oldest white dwarf planetary systems; 43. What does the chemical composition of giant planets tells us about their formation?; 44. Chemical characterization of exoplanetary atmospheres; 45. JWST: the role of observing facilities in setting the agenda; 46. ALMA Band 1 and astrochemistry; 47. ALMA; 48. Processing of interstellar ices by soft X-rays and swift ions; 49. Laboratory measurements of methanol photolysis branching ratios to guide astrochemical models; 50. Acetaldehyde and carbonaceous dust; 51. Photodestruction of astrophysically relevant ice species; 52. Synchrotron X-ray irradiation of N-rich organics; 53. Gas phase studies of astrochemical importance; 54. Photochemistry and radiation chemistry of cosmic ice analogs of ammonia.