133 related articles for article (PubMed ID: 11539404)
1. Variations in the 3 micron spectrum across the Orion Bar: polycyclic aromatic hydrocarbons and related molecules.
Sloan GC; Bregman JD; Geballe TR; Allamandola LJ; Woodward CE
Astrophys J; 1997 Jan; 474(2 Pt 1):735-40. PubMed ID: 11539404
[TBL] [Abstract][Full Text] [Related]
2. Peripherally hydrogenated neutral polycyclic aromatic hydrocarbons as carriers of the 3 micron interstellar infrared emission complex: results from single-photon infrared emission spectroscopy.
Wagner DR; Kim HS; Saykally RJ
Astrophys J; 2000 Dec; 545(2 Pt 1):854-60. PubMed ID: 11878349
[TBL] [Abstract][Full Text] [Related]
3. Spatial variations of the 3 micron emission features within UV-excited nebulae: photochemical evolution of interstellar polycyclic aromatic hydrocarbons.
Geballe TR; Tielens AG; Allamandola LJ; Moorhouse A; Brand PW
Astrophys J; 1989 Jun; 341(1 Pt 1):278-87. PubMed ID: 11542168
[TBL] [Abstract][Full Text] [Related]
4. The discovery of a new infrared emission feature at 1905 wavenumbers (5.25 microns) in the spectrum of BD +30 degrees 3639 and its relation to the polycyclic aromatic hydrocarbon model.
Allamandola LJ; Bregman JD; Sandford SA; Tielens AG; Witteborn FC; Wooden DH; Rank D
Astrophys J; 1989 Oct; 345(1):L59-62. PubMed ID: 11538325
[TBL] [Abstract][Full Text] [Related]
5. Hydrogenated polycyclic aromatic hydrocarbons and the 2940 and 2850 wavenumber (3.40 and 3.51 micron) infrared emission features.
Bernstein MP; Sandford SA; Allamandola LJ
Astrophys J; 1996 Dec; 472(2):L127-30. PubMed ID: 11541245
[TBL] [Abstract][Full Text] [Related]
6. The infrared emission bands. II. A spatial and spectral study of the Orion Bar.
Bregman JD; Allamandola LJ; Tielens AG; Geballe TR; Witteborn FC
Astrophys J; 1989 Sep; 344(2):791-8. PubMed ID: 11538351
[TBL] [Abstract][Full Text] [Related]
7. New emission features in the 11-13 micron region and their relationship to polycyclic aromatic hydrocarbons.
Witteborn FC; Sandford SA; Bregman JD; Allamandola LJ; Cohen M; Wooden DH; Graps AL
Astrophys J; 1989 Jun; 341(1):270-7. PubMed ID: 11542169
[TBL] [Abstract][Full Text] [Related]
8. Spatial variation of the 3.29 and 3.40 micron emission bands within reflection nebulae and the photochemical evolution of methylated polycyclic aromatic hydrocarbons.
Joblin C; Tielens AG; Allamandola LJ; Geballe TR
Astrophys J; 1996 Feb; 458(2 Pt 1):610-20. PubMed ID: 11538557
[TBL] [Abstract][Full Text] [Related]
9. The anomalous 3.43 and 3.53 micron emission features toward HD 97048 and Elias 1: C-C vibrational modes of polycyclic aromatic hydrocarbons?
Schutte WA; Tielens AG; Allamandola LJ; Cohen M; Wooden DH
Astrophys J; 1990 Sep; 360(2 Pt 1):577-89. PubMed ID: 11538697
[TBL] [Abstract][Full Text] [Related]
10. Assessment of the polycyclic aromatic hydrocarbon-diffuse interstellar band proposal.
Salama F; Bakes EL; Allamandola LJ; Tielens AG
Astrophys J; 1996 Feb; 458(2 Pt 1):621-36. PubMed ID: 11538558
[TBL] [Abstract][Full Text] [Related]
11. Interstellar polycyclic aromatic hydrocarbons: the infrared emission bands, the excitation/emission mechanism, and the astrophysical implications.
Allamandola LJ; Tielens AG; Barker JR
Astrophys J Suppl Ser; 1989 Dec; 71():733-75. PubMed ID: 11542189
[TBL] [Abstract][Full Text] [Related]
12. Infrared spectroscopy of dense clouds in the C-H stretch region: methanol and "diamonds.".
Allamandola LJ; Sandford SA; Tielens AG; Herbst TM
Astrophys J; 1992 Nov; 399():134-46. PubMed ID: 11540063
[TBL] [Abstract][Full Text] [Related]
13. A laboratory analog for the carrier of the 3 micron emission of the protoplanetary nebula IRAS 05341+0852.
Beegle LW; Wdowiak TJ; Arnoult KM
Astrophys J; 1997 Sep; 486(2):L153-5. PubMed ID: 11540593
[TBL] [Abstract][Full Text] [Related]
14. Simulated infrared emission spectra of highly excited polyatomic molecules: a detailed model of the PAH-UIR hypothesis.
Cook DJ; Saykally RJ
Astrophys J; 1998 Feb; 493 Pt 1(2):793-802. PubMed ID: 11541733
[TBL] [Abstract][Full Text] [Related]
15. The spacing of the interstellar 6.2 and 7.7 micron emission features as an indicator of polycyclic aromatic hydrocarbon size.
Hudgins DM; Allamandola LJ
Astrophys J; 1999 Mar; 513(1 Pt 2):L69-73. PubMed ID: 11543062
[TBL] [Abstract][Full Text] [Related]
16. The infrared emission bands. III. Southern IRAS sources.
Cohen M; Tielens AG; Bregman J; Witteborn FC; Rank DM; Allamandola LJ; Wooden DH; de Muizon M
Astrophys J; 1989 Jun; 341(1 Pt 1):246-69. PubMed ID: 11542167
[TBL] [Abstract][Full Text] [Related]
17. Insoluble organic material of the Orgueil carbonaceous chondrite and the unidentified infrared bands.
Wdowiak TJ; Flickinger GC; Cronin JR
Astrophys J; 1988 May; 328(2):L75-9. PubMed ID: 11538467
[TBL] [Abstract][Full Text] [Related]
18. The 2.5-12 micrometers spectrum of comet Halley from the IKS-VEGA experiment.
Combes M; Moroz VI; Crovisier J; Encrenaz T; Bibring JP; Grigoriev AV; Sanko NF; Coron N; Crifo JF; Gispert R; Bockelée-Morvan D; Nikolsky YuV ; Krasnopolsky VA; Owen T; Emerich C; Lamarre JM; Rocard F
Icarus; 1988; 76():404-36. PubMed ID: 11538667
[TBL] [Abstract][Full Text] [Related]
19. Infrared spectroscopy of matrix-isolated polycyclic aromatic hydrocarbon cations. 2. The members of the thermodynamically most favorable series through coronene.
Hudgins DM; Allamandola LJ
J Phys Chem; 1995 Mar; 99(10):3033-46. PubMed ID: 11538457
[TBL] [Abstract][Full Text] [Related]
20. Laboratory investigation of the contribution of complex aromatic/aliphatic polycyclic hybrid molecular structures to interstellar ultraviolet extinction and infrared emission.
Arnoult KM; Wdowiak TJ; Beegle LW
Astrophys J; 2000 Jun; 535(2 Pt 1):815-22. PubMed ID: 11543517
[TBL] [Abstract][Full Text] [Related]
[Next] [New Search]