
UvA-DARE (Digital Academic Repository) The hidden life of cosmic carbon Infrared fingerprint spectroscopy and fragmentation chemistry of gas-phase polycyclic aromatic hydrocarbons Wiersma, S.D. Publication date 2021 License Other Link to publication Citation for published version (APA): Wiersma, S. D. (2021). The hidden life of cosmic carbon: Infrared fingerprint spectroscopy and fragmentation chemistry of gas-phase polycyclic aromatic hydrocarbons. General rights It is not permitted to download or to forward/distribute the text or part of it without the consent of the author(s) and/or copyright holder(s), other than for strictly personal, individual use, unless the work is under an open content license (like Creative Commons). Disclaimer/Complaints regulations If you believe that digital publication of certain material infringes any of your rights or (privacy) interests, please let the Library know, stating your reasons. In case of a legitimate complaint, the Library will make the material inaccessible and/or remove it from the website. Please Ask the Library: https://uba.uva.nl/en/contact, or a letter to: Library of the University of Amsterdam, Secretariat, Singel 425, 1012 WP Amsterdam, The Netherlands. You will be contacted as soon as possible. UvA-DARE is a service provided by the library of the University of Amsterdam (https://dare.uva.nl) Download date:28 Sep 2021 Bibliography 1. Clemens, D. P., Yun, J. L. & Heyer, M. H. Bok globules and small molecular clouds - Deep IRAS photometry and (C-12)O spectroscopy. Astrophys. J. Suppl. Ser. 75, 877–904 (1991). 2. Murray, N. Star formation efficiencies and lifetimes of giant molecular clouds in the Milky Way. Astrophys. J. 729, 133 (2011). 3. Hollenbach, D. J. & Tielens, A. G. G. M. Photodissociation regions in the interstellar medium of galaxies. Rev. Mod. Phys. 71, 173–230 (1999). 4. Greenwood, N. N. & Earnshaw, A. Chemistry of the elements 2nd ed., 4 (Butterworth- Heinemann, 1997). 5. Ostlie, D. A. & Carroll, B. W. An Introduction to Modern Stellar Astrophysics 1st ed. (Ben- jamin Cummings, 1995). 6. Henning, T. & Salama, F. Carbon in the Universe. Science 282, 2204–2210 (1998). 7. Tielens, A. G. G. M. The Physics and Chemistry of the Interstellar Medium 1st ed., 495 (Cambridge University Press, 2005). 8. Müller, H. S. P., Schlöder, F., Stutzki, J. & Winnewisser, G. The Cologne Database for Molec- ular Spectroscopy, CDMS: A useful tool for astronomers and spectroscopists. J. Mol. Struct. 742, 215–227. https://cdms.astro.uni-koeln.de/classic/molecules (2005). 9. Karakas, A. I. & Lattanzio, J. C. AGB Stars and the Observed Abundance of Neon in Plane- tary Nebulae. Publ. Astron. Soc. Aust. 20, 393–400 (2003). 10. Woosley, S. E., Heger, A. & Weaver, T. A. The evolution and explosion of massive stars. Rev. Mod. Phys. 74, 1015–1071 (2002). 11. Fraknoi A.and Morrison, D. & Wolff, S. C. Astronomy https://openstax.org/details/ books/astronomy (OpenStax, Rice University, Houston, 2018). 12. Ehrenfreund, P. & Menten, K. M. in Astrobiology (eds Horneck, G. & Baumstark-Khan, C.) 1, 7–23 (Springer Berlin Heidelberg, 2002). 13. Wood, P. R., Olivier, E. A. & Kawaler, S. D. Long Secondary Periods in Pulsating Asymp- totic Giant Branch Stars: An Investigation of Their Origin. Astrophys. J. 604, 800–816 (2004). 14. Tielens, A. G. G. M. Photodissociation Regions and Planetary Nebulae. Symp. - Int. Astron. Union 155, 155–162 (1993). 15. Tielens, A. G. G. M. The molecular universe. Rev. Mod. Phys. 85, 1021–1081 (2013). 16. Albertsson, T., Semenov, D. A., Vasyunin, A. I., Henning, T. & Herbst, E. New extended deuterium fractionation model: Assessment at dense ISM conditions and sensitivity analysis. Astrophys. J. Suppl. Ser. 207, 27 (2013). 129 Bibliography 17. Draine, B. T. Can Dust Explain Variations in the D/H Ratio? in Astrophysics in the Far Ul- traviolet, Five Years of Discovery with FUSE: Astronomical Society of the Pacific Conference Series (eds Sonneborn, G., Moos, H. & Andersson, B.-G.) 348 (2006), 58. 18. Linsky, J. L. et al. What Is the Total Deuterium Abundance in the Local Galactic Disk? Astrophys. J. 647, 1106–1124 (2006). 19. Roueff, E., Herbst, E., Lis, D. C. & Phillips, T. G. The Effect of an Increased Elemental D/H Ratio on Deuterium Fractionation in the Cold Interstellar Medium. Astrophys. J. 661, L159–L162 (2007). 20. Cazaux, S., Caselli, P. & Spaans, M. Interstellar ices as witnesses of star formation: Selective deuteration of water and organic molecules unveiled. Astrophys. J. Lett. 741, L34 (2011). 21. Lamberts, T., Samanta, P. K., Köhn, A. & Kästner, J. Quantum tunneling during interstellar surface-catalyzed formation of water: the reaction H + H2O2 −−! H2O + OH. Phys. Chem. Chem. Phys. 18, 33021–33030 (2016). 22. Kerridge, J. F., Chang, S. & Shipp, R. Isotopic characterisation of kerogen-like material in the Murchison carbonaceous chondrite. Geochim. Cosmochim. Acta 51, 2527–2540 (1987). 23. Laurent, B. et al. The deuterium/hydrogen distribution in chondritic organic matter attests to early ionizing irradiation. Nat. Commun. 6, 8567 (2015). 24. Remusat, L., Piani, L. & Bernard, S. Thermal recalcitrance of the organic D-rich component of ordinary chondrites. Earth Planet. Sci. Lett. 435, 36–44 (2016). 25. Hersant, F., Gautier, D. & Hure, J. A Two-dimensional Model for the Primordial Nebula Constrained by D/H Measurements in the Solar System: Implications for the Formation of Giant Planets. Astrophys. J. 554, 391–407 (2001). 26. Hartogh, P. et al. Ocean-like water in the Jupiter-family comet 103P/Hartley 2. Nature 478, 218–220 (2011). 27. Swings, P. & Rosenfeld, L. Considerations Regarding Interstellar Molecules. Astrophys. J. 86, 483 (1937). 28. Russell, H. N. The Analysis of Spectra and its Applications in Astronomy. Mon. Not. R. Astron. Soc. 95, 610–636 (1935). 29. Cami, J., Bernard-Salas, J., Peeters, E. & Malek, S. E. Detection of C60 and C70 in a Young Planetary Nebula. Science 329, 1180–1182 (2010). + 30. Campbell, E. K., Holz, M., Gerlich, D. & Maier, J. P. Laboratory confirmation of C60 as the carrier of two diffuse interstellar bands. Nature 523, 322–323 (2015). 31. Kroto, H. W., Heath, J. R., O’Brien, S. C., Curl, R. F. & Smalley, R. E. C60: Buckminster- fullerene. Nature 318, 162–163 (1985). 32. Peeters, E. The PAH Hypothesis after 25 Years. Proc. Int. Astron. Union 7, 149–161 (2011). 33. Rieke, G. H. History of infrared telescopes and astronomy. Exp. Astron. 25, 125–141 (2009). 34. Gillett, F. C., Forrest, W. J. & Merrill, K. M. 8–13 micron spectra of NGC 7027, BD+30°3639 and NGC 6572. Astrophys. J. 183, 87 (1973). 35. Russell, R. W., Soifer, B. T. & Willner, S. P. The infrared spectra of CRL 618 and HD 44179 (CRL 915). Astrophys. J. 220, 568 (1978). 130 Bibliography 36. Sellgren, K. The near-infrared continuum emission of visual reflection nebulae. Astrophys. J. 277, 623 (1984). 37. Leger, A. & Puget, J. L. Identification of the unidentified IR emission features of interstellar dust? Astron. Astrophys. 137, L5–L8 (1984). 38. Allamandola, L. J., Tielens, A. G. G. M. & Barker, J. R. Polycyclic aromatic hydrocarbons and the unidentified infrared emission bands - Auto exhaust along the Milky Way. Astrophys. J. 290, L25 (1985). 39. Draine, B. T. Interstellar Dust Grains. Annu. Rev. Astron. Astrophys. 41, 241–289 (2003). 40. Joblin, C., Leger, A. & Martin, P. Contribution of polycyclic aromatic hydrocarbon molecules to the interstellar extinction curve. Astrophys. J. 393, L79 (1992). 41. Li, A. & Draine, B. T. Infrared Emission from Interstellar Dust. II. The Diffuse Interstellar Medium. Astrophys. J. 554, 778–802 (2001). 42. Mulas, G., Malloci, G., Joblin, C. & Cecchi-Pestellini, C. Polycyclic aromatic hydrocarbons and the extinction curve in EAS Publications Series 46 (2011), 327–340. 43. Allamandola, L. J., Tielens, G. G. M. & Barker, J. R. Interstellar polycyclic aromatic hydro- carbons - The infrared emission bands, the excitation/emission mechanism, and the astro- physical implications. Astrophys. J. Suppl. Ser. 71, 733–775 (1989). 44. Allain, T., Leach, S. & Sedlmayr, E. Photodestruction of PAHs in the interstellar medium. II. Influence of the states of ionization and hydrogenation. Astron. Astrophys. 305, 616 (1996). 45. Li, A. & Draine, B. T. The carriers of the interstellar unidentified infrared emission features: Aromatic or aliphatic? Astrophys. J. Lett. 760, L35 (2012). 46. Yang, X. J., Li, A., Glaser, R. & Zhong, J. X. Polycyclic Aromatic Hydrocarbons with Aliphatic Sidegroups: Intensity Scaling for the C–H Stretching Modes and Astrophysical Implications. Astrophys. J. 837, 171 (2017). 47. Tielens, A. G. G. M. Interstellar Polycyclic Aromatic Hydrocarbon Molecules. Annu. Rev. Astron. Astrophys. 46, 289–337 (2008). 48. Desert, F. X., Boulanger, F. & Puget, J. L. Interstellar dust models for extinction and emis- sion. Astron. Astrophys. 237, 215–236 (1990). 49. Schutte, W. A., Tielens, A. G. G. M. & Allamandola, L. J. Theoretical modeling of the infrared fluorescence from interstellar polycyclic aromatic hydrocarbons. Astrophys. J. 415, 397 (1993). 50. Ricca, A., Bauschlicher, C. W., Boersma, C., Tielens, A. G. G. M. & Allamandola, L. J. The Infrared Spectroscopy of Compact Polycyclic Aromatic Hydrocarbons Containing up to 384 Carbons. Astrophys. J. 754, 75 (2012). 51. Andrews, H. et al. PAH emission at the bright locations of PDRs: The grandPAH hypothesis. Astrophys. J. 807, 99 (2015). 52. Rapacioli, M., Joblin, C. & Boissel, P. Spectroscopy of polycyclic aromatic hydrocarbons and very small grains in photodissociation regions. Astron. Astrophys. 429, 193–204 (2005). 53. Berné, O. et al. Extended Red Emission and the evolution of carbonaceous nanograins in NGC 7023. Astron. Astrophys. 479, L41–L44 (2008). 131 Bibliography 54. Mulas, G., Malloci, G., Joblin, C. & Toublanc, D. Diagnostics for specific PAHs in the far- IR: searching neutral naphthalene and anthracene in the Red Rectangle. Astron. Astrophys. 456, 161–169 (2006). 55. Mulas, G., Malloci, G., Joblin, C. & Toublanc, D. A general model for the identification of specific PAHs in the far-IR.
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