About the chemical composition of carriers of the unidentified infrared bands (UIBs) and protoplanetary emission spectra recorded from certain astronomical objects

European Space Agency, (Special Publication) ESA SP

Volumn , Issue 518, 2002, Pages 439-440

  Cataldo, Franco ^a   Keheyan, Yeghis ^b   Heymann, Dieter ^c  

^a Soc Lupi Chem Research Institute   (Italy)

^b SAPIENZA UNIVERSITY OF ROME   (Italy)

^c RICE UNIVERSITY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

COMPOSITION EFFECTS; INFRARED RADIATION; MOLECULES; POLYCYCLIC AROMATIC HYDROCARBONS; SPACE RESEARCH;

ASTRONOMICAL OBJECTS;

ASTROPHYSICS;

EID: 0036766127     PISSN: 03796566     EISSN: None     Source Type: Conference Proceeding    
DOI: None     Document Type: Conference Paper

References (3)

1. F.Cataldo, Y. Keheyan and D. Heymann. A new model for the interpretation of the unidentified infrared bands (UIBs) of the interstellar medium and of the protoplanetary nebulae, INTERNATIONAL JOURNAL OF ASTROBIOLOGY, Vol.1, in press, 2002.
2. Reinaud C., et al. Optical Properties of synthetic carbon nanoparticles as model of cosmic dust. SPECTROCHIMICA ACTA, Vol. A57, 797-814 2001.
3. Hayatsu R., Anders E. Organic compounds in meteorites and their origins. TOPICS IN CURRENT CHEMISTRY, Vol. 99, 1-37, 1981.