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1-12
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Results: 12
Authors:
Hony, S
Van Kerckhoven, C
Peeters, E
Tielens, AGGM
Hudgins, DM
Allamandola, LJ
Citation: S. Hony et al., The CH out-of-plane bending modes of PAH molecules in astrophysical environments, ASTRON ASTR, 370(3), 2001, pp. 1030-1043
Authors:
Hudgins, DM
Bauschlicher, CW
Allamandola, LJ
Citation: Dm. Hudgins et al., Closed-shell polycyclic aromatic hydrocarbon cations: a new category of interstellar polycyclic aromatic hydrocarbons, SPECT ACT A, 57(4), 2001, pp. 907-930
Authors:
Bakes, ELO
Tielens, AGGM
Bauschlicher, CW
Hudgins, DM
Allamandola, LJ
Citation: Elo. Bakes et al., Theoretical modeling of infrared emission from neutral and charged polycyclic aromatic hydrocarbons. II., ASTROPHYS J, 560(1), 2001, pp. 261-271
Authors:
Halasinski, TM
Hudgins, DM
Salama, F
Allamandola, LJ
Bally, T
Citation: Tm. Halasinski et al., Electronic absorption spectra of neutral pentacene (C22H14) and its positive and negative ions in Ne, Ar, and Kr matrices, J PHYS CH A, 104(32), 2000, pp. 7484-7491
Authors:
Hudgins, DM
Bauschlicher, CW
Allamandola, LJ
Fetzer, JC
Citation: Dm. Hudgins et al., Infrared spectroscopy of matrix-isolated polycyclic aromatic hydrocarbon ions. 5. PAHs incorporating a cyclopentadienyl ring, J PHYS CH A, 104(16), 2000, pp. 3655-3669
Authors:
Van Kerckhoven, C
Hony, S
Peeters, E
Tielens, AGGM
Allamandola, LJ
Hudgins, DM
Cox, P
Roelfsema, PR
Voors, RHM
Waelkens, C
Waters, LBFM
Wesselius, PR
Citation: C. Van Kerckhoven et al., The C-C-C bending modes of PAHs: a new emission plateau from 15 to 20 mu m, ASTRON ASTR, 357(3), 2000, pp. 1013-1019
Authors:
Bauschlicher, CW
Hudgins, DM
Allamandola, LJ
Citation: Cw. Bauschlicher et al., The infrared spectra of polycyclic aromatic hydrocarbons containing a five-membered ring: symmetry breaking and the B3LYP functional, THEOR CH AC, 103(2), 1999, pp. 154-162
Authors:
Hudgins, DM
Allamandola, LJ
Citation: Dm. Hudgins et Lj. Allamandola, Interstellar PAH emission in the 11-14 micron region: New insights from laboratory data and a tracer of ionized PAHs, ASTROPHYS J, 516(1), 1999, pp. L41-L44
Direct spectroscopic evidence for ionized polycyclic aromatic hydrocarbonsin the interstellar medium
Authors:
Sloan, GC
Hayward, TL
Allamandola, LJ
Bregman, JD
DeVito, B
Hudgins, DM
Citation: Gc. Sloan et al., Direct spectroscopic evidence for ionized polycyclic aromatic hydrocarbonsin the interstellar medium, ASTROPHYS J, 513(1), 1999, pp. L65-L68
Authors:
Hudgins, DM
Allamandola, LJ
Citation: Dm. Hudgins et Lj. Allamandola, The spacing of the interstellar 6.2 and 7.7 micron emission features as anindicator of polycyclic aromatic hydrocarbon size, ASTROPHYS J, 513(1), 1999, pp. L69-L73
Authors:
Allamandola, LJ
Hudgins, DM
Sandford, SA
Citation: Lj. Allamandola et al., Modeling the unidentified infrared emission with combinations of polycyclic aromatic hydrocarbons, ASTROPHYS J, 511(2), 1999, pp. L115-L119
Authors:
Allamandola, LJ
Hudgins, DM
Bauschlicher, CW
Langhoff, SR
Citation: Lj. Allamandola et al., Carbon chain abundance in the diffuse interstellar medium, ASTRON ASTR, 352(2), 1999, pp. 659-664
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