Hexa-peri-benzocoronene, a candidate for the origin of the diffuse interstellar visible absorption bands ?

Tetrahedron

Volumn 42, Issue 4, 1986, Pages 1127-1134

  Hendel, W ^a   Khan, Z H ^a,c   Schmidt, W ^a,b  

^a UNIVERSITY OF ERLANGEN NUREMBERG   (Germany)

^b Biochemisches Institut für Umweltcarcinogene ^*  (Germany)

^c JAMIA MILLIA ISLAMIA CENTRAL UNIVERSITY   (India)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0001590255     PISSN: 00404020     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0040-4020(01)87517-7     Document Type: Article

References (35)

1. The diffuse interstellar bands. IV - The region 4400-6850 A
2. Interstellar grains The interaction of light with a small-particle system
3. Distinction Between Models of Interstellar Grains
4. On the Optical Properties of Interstellar Dust.
5. Polycyclic Hydrocarbons, Platt Particles, and Interstellar Extinction
6. 378. 1 : 12-2 : 3-10 : 11-Tribenzoperylene
7. 28. The electronic interaction between benzenoid rings in condensed aromatic hydrocarbons. 1 : 12-2 : 3-4 : 5-6 : 7-8 : 9-10 : 11-hexabenzocoronene, 1 : 2-3 : 4-5 : 6-10 : 11-tetrabenzoanthanthrene, and 4 : 5-6 : 7-11 : 12-13 : 14-tetrabenzoperopyrene
8. Anthraquinones Complètement Substituées et Anthracènes Correspondants: I. Composés Substitués Symétriquement
9. Discovery of optical molecular emission from the bipolar nebula surrounding HD 44179
10. Photoelectron spectra of polynuclear aromatics. III. The effect of nonplanarity in sterically overcrowded aromatic hydrocarbons