Experimental indication of a naphthalene-base molecular aggregate for the carrier of the 2175 angstrom interstellar extinction feature

被引:33
作者
Beegle, LW
Wdowiak, TJ
Robinson, MS
Cronin, JR
McGehee, MD
Clemett, SJ
Gillette, S
机构
[1] ARIZONA STATE UNIV,DEPT CHEM & BIOCHEM,TEMPE,AZ 85287
[2] STANFORD UNIV,DEPT CHEM,PALO ALTO,CA 94305
关键词
dust; extinction; infrared; ISM; lines and bands; molecules methods; laboratory; molecular processes; ultraviolet;
D O I
10.1086/304658
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Experiments where the simple polycyclic aromatic hydrocarbon (PAH) naphthalene (C10H8) is subjected to the energetic environment of a plasma have resulted in the synthesis of a molecular aggregate that has ultraviolet spectral characteristics that suggest it provides insight into the nature of the carrier of the 2175 Angstrom interstellar extinction feature and may be a laboratory analog. Ultraviolet, visible, infrared, and mass spectroscopy, along with gas chromatography, indicate that it is a molecular aggregate in which an aromatic double ring (''naphthaalene'') structural base serves as the electron ''box'' chromophore that gives rise to the envelope of the 2175 Angstrom feature. This chromophore can also provide the peak of the feature or function as a mantle in concert with another peak provider such as graphite. The molecular base/chromophore manifests itself both as a structural component of an alkyl-aromatic polymer and as a substructure of hydrogenated PAH species. Its spectral and molecular characteristics are consistent with what is generally expected for a complex molecular aggregate that has a role as an interstellar constituent.
引用
收藏
页码:976 / 982
页数:7
相关论文
共 37 条
[1]   INTERSTELLAR POLYCYCLIC AROMATIC-HYDROCARBONS - THE INFRARED-EMISSION BANDS, THE EXCITATION EMISSION MECHANISM, AND THE ASTROPHYSICAL IMPLICATIONS [J].
ALLAMANDOLA, LJ ;
TIELENS, AGGM ;
BARKER, JR .
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1989, 71 (04) :733-775
[2]  
BEEGLE LW, 1997, THESIS U ALABAMA BIR
[3]   Hydrogenated polycyclic aromatic hydrocarbons and the 2940 and 2850 wavenumber (3.40 and 3.51 micron) infrared emission features [J].
Bernstein, MP ;
Sandford, SA ;
Allamandola, LJ .
ASTROPHYSICAL JOURNAL, 1996, 472 (02) :L127-L130
[4]   Carbon grains produced in partially hydrogenated atmospheres and their astrophysical relevance [J].
Blanco, A ;
Fonti, S ;
Muci, AM ;
Orofino, V .
ASTROPHYSICAL JOURNAL, 1996, 472 (01) :419-423
[5]   ULTRAVIOLET PHOTOMETRY FROM ORBITING ASTRONOMICAL OBSERVATORY .2. INNERSTELLAR EXTINCTION [J].
BLESS, RC ;
SAVAGE, BD .
ASTROPHYSICAL JOURNAL, 1972, 171 (02) :293-&
[6]  
Draine B. T., 1989, IAU S, V135, P313
[7]   AN ANALYSIS OF THE SHAPES OF ULTRAVIOLET EXTINCTION CURVES .1. THE 2175-A BUMP [J].
FITZPATRICK, EL ;
MASSA, D .
ASTROPHYSICAL JOURNAL, 1986, 307 (01) :286-294
[8]  
GEBALLE TR, 1990, ASTRON ASTROPHYS, V235, pL9
[9]  
Huffman D., 1989, IAU S, V135, P329
[10]   Spatial variation of the 3.29 and 3.40 micron emission bands within reflection nebulae and the photochemical evolution of methylated polycyclic aromatic hydrocarbons [J].
Joblin, C ;
Tielens, AGGM ;
Allamandola, LJ ;
Geballe, TR .
ASTROPHYSICAL JOURNAL, 1996, 458 (02) :610-620