![]() ![]() Įngelbracht CW, Kundurthy KD, Gordon KD et al (2006) Extended mid-infrared aromatic feature emission in M82. ĭuley WW, Williams DA (1981) The infrared spectrum of interstellar dust – surface functional groups on carbon. ĭraine BT, Lazarian A (1998) Electric dipole radiation from spinning dust grains. ĭoney KD, Candian A, Mori T, Onaka T, Tielens AGGM (2016) Deuterated polycyclic aromatic hydrocarbons: revisited. Ĭroiset BA, Candian A, Berné O, Tielens AGGM (2016) Mapping PAH sizes in NGC7023 with SOFIA. Ĭernicharo J, Agúndez M, Cabezas C, Tercero B, Marcelino N, Pardo JR, de Vicente P (2021) Pure hydrocarbon cycles in TMC-1: discovery of ethynyl cyclopropenylidene, cyclopentadiene and indene. Ĭandian A, Kerr TH, Song I-O, McCombie J, Sarre PJ (2012) Spatial distribution and interpretation of the 3.3 μm PAH emission band of the red rectangle. Ĭampbell EK, Holz M, Gerlich D, Maier JP (2015) Laboratory confirmation of C60+ as the carrier of two diffuse interstellar bands. Ĭami J, Bernard-Salas J, Peeters E, Malek SE (2010) Detection of C60 and C70 in a young planetary nebula. Ĭami J, Cox N (eds) (2014) Proceedings of IAU symposium 297: diffuse interstellar bands. Ĭalzetti D (2020) Star formation in galaxies as traced by the Spitzer space telescope. īurkhardt AM, Lee KLK, Changala PB et al (2021) Discovery of the pure polycyclic aromatic hydrocarbon indene ($c$-C$_9$H$_8$) with GOTHAM observations of TMC-1. īoersma C, Bauschlicher CW, Ricca A, Mattioda AL, Cami J, Peeters E, Sánchez de Armas F, Puerta Saborido G, Hudgins DM, Allamandola LJ (2014) The NASA Ames PAH IR spectroscopic database version 2.00: updated content, web site, and on(off)line tools. PAH size, charge, composition, and structure. īoersma C, Bregman JD, Allamandola LJ (2013) Properties of polycyclic aromatic hydrocarbons in the northwest photon dominated region of NGC 7023. īoersma C (2009) PhD thesis, University of Groningenīoersma C, Bouwman J, Lahuis F et al (2008) The characteristics of the IR emission features in the spectra of Herbig Ae stars: evidence for chemical evolution. īernstein MP, Sandford SA, Allamandola LJ, Gillette JS, Clemett SJ, Zare RN (1999) UV irradiation of polycyclic aromatic hydrocarbons in ices: production of alcohols, quinones, and ethers. īerné O, Fuente A, Goicoechea JR et al (2009) Mid-infrared polycyclic aromatic hydrocarbon and H 2 emission as a probe of physical conditions in extreme photodissociation regions. Wiley, New Yorkīerné O, Tielens AGGM (2015) Formation of buckminsterfullerene (C60) in interstellar space. īellamy L (1958) The infra-red spectra of complex molecules, 2nd edn. īauschlicher CW, Ricca A, Boersma C, Allamandola LJ (2018) The NASA Ames PAH IR spectroscopic database: computational version 3.00 with updated content and the introduction of multiple scaling factors. īauschlicher CW, Boersma C, Ricca A et al (2010) The NASA Ames polycyclic aromatic hydrocarbon infrared spectroscopic database: the computed spectra. ![]() īauschlicher CW Jr, Peeters E, Allamandola LJ (2009) The infrared spectra of very large irregular polycyclic aromatic hydrocarbons (PAHs): observational probes of astronomical PAH geometry, size, and charge. ![]() īauschlicher CW Jr, Peeters E, Allamandola LJ (2008) The infrared spectra of very large, compact, highly symmetric, polycyclic aromatic hydrocarbons (PAHs). Īndrews H, Boersma C, Werner MW, Livingston J, Allamandola LJ, Tielens AGGM (2015) PAH emission at the bright locations of PDRs: the grandPAH hypothesis. Allamandola LJ, Tielens AGGM, Barker JR (1989) Interstellar polycyclic aromatic hydrocarbons – the infrared emission bands, the excitation/emission mechanism, and the astrophysical implications.
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