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
[11]  
KELLER R, 1987, POLYCYCL AROMAT COMP, P387
[12]   LABORATORY SPECTRA OF POLYCYCLIC AROMATIC HYDROCARBON IONS AND THE INTERSTELLAR EXTINCTION CURVE [J].
LEE, W ;
WDOWIAK, TJ .
ASTROPHYSICAL JOURNAL, 1993, 410 (02) :L127-L130
[13]   INTERSTELLAR DUST AND EXTINCTION [J].
MATHIS, JS .
ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1990, 28 :37-70
[14]   THE ORIGIN OF VARIATIONS IN THE 2175 ANGSTROM EXTINCTION BUMP [J].
MATHIS, JS .
ASTROPHYSICAL JOURNAL, 1994, 422 (01) :176-186
[15]   Activation of an ultraviolet resonance in hydrogenated amorphous carbon grains by exposure to ultraviolet radiation [J].
Mennella, V ;
Colangeli, L ;
Palumbo, P ;
Rotundi, A ;
Schutte, W ;
Bussoletti, E .
ASTROPHYSICAL JOURNAL, 1996, 464 (02) :L191-L194
[16]   ULTRAVIOLET INTER-STELLAR EXTINCTION TOWARD 1367 STARS OBSERVED BY ANS [J].
MEYER, DM ;
SAVAGE, BD .
ASTROPHYSICAL JOURNAL, 1981, 248 (02) :545-562
[17]   PHENYLMALEIC ANHYDRIDE AS A DIENE IN THE DIELS-ALDER REACTION [J].
MILLER, LE ;
MANN, DJ .
JOURNAL OF THE AMERICAN CHEMICAL SOCIETY, 1951, 73 (01) :45-48
[18]  
MURRELL JN, 1963, THEORY ELECT SPECTRA, P93
[19]  
NANDY K, 1976, ASTRON ASTROPHYS, V51, P63
[20]  
NANDY K, 1975, ASTRON ASTROPHYS, V44, P195