GAS-PHASE ELECTRONIC SPECTRA OF CARBON-CHAIN RADICALS COMPARED WITH DIFFUSE INTERSTELLAR BAND OBSERVATIONS Export

@article{citeulike:4182329, abstract = {This paper compares laboratory gas-phase spectra of neutral and cationic linear carbon-chain radicals with astronomical di†use interstellar band (DIB) spectra. The origin bands of the strong electronic transitions of the studied species, C (n\3\`{E}6), (n\2\`{E}4), (n\3, 4), do not coincide 2nH HC2nH` NC2n\~{}2N` with detectable DIBs, except for HC (n\3), which possibly matches a weak feature. It is con- 2n\~{}1N` cluded that the column densities of these species through the observed di†use clouds are below 2]1012 cm\~{}2. The proÐle change and the shift of the maxima of the absorption bands with temperature are illustrated. The relation to radio-astronomical detection of carbon chains in di†use media is also discussed.}, author = {Motylewski, T. and Linnartz, H. and Vaizert, O. and Maier, J. P. and Galazutdinov, G. A. and Musaev, F. A. and Krebowski, J. and Walker, G. A. H. and Bohlender, D. A.}, citeulike-article-id = {4182329}, citeulike-linkout-0 = {http://www.iop.org/EJ/article/0004-637X/531/1/312/50370.web.pdf?request-id=e0cead8e-2f13-45ec-8329-7f3d297b8c88}, keywords = {and, bands, ism, lines, molecules}, posted-at = {2009-03-16 14:32:30}, priority = {2}, title = {GAS-PHASE ELECTRONIC SPECTRA OF CARBON-CHAIN RADICALS COMPARED WITH DIFFUSE INTERSTELLAR BAND OBSERVATIONS}, url = {http://www.iop.org/EJ/article/0004-637X/531/1/312/50370.web.pdf?request-id=e0cead8e-2f13-45ec-8329-7f3d297b8c88}, year = {2000} }

TY - JOUR ID - citeulike:4182329 L3 - citeulike-article-id:4182329 N2 - This paper compares laboratory gas-phase spectra of neutral and cationic linear carbon-chain radicals with astronomical di†use interstellar band (DIB) spectra. The origin bands of the strong electronic transitions of the studied species, C (n\3È6), (n\2È4), (n\3, 4), do not coincide 2nH HC2nH` NC2n~2N` with detectable DIBs, except for HC (n\3), which possibly matches a weak feature. It is con- 2n~1N` cluded that the column densities of these species through the observed di†use clouds are below 2]1012 cm~2. The proÐle change and the shift of the maxima of the absorption bands with temperature are illustrated. The relation to radio-astronomical detection of carbon chains in di†use media is also discussed. TI - GAS-PHASE ELECTRONIC SPECTRA OF CARBON-CHAIN RADICALS COMPARED WITH DIFFUSE INTERSTELLAR BAND OBSERVATIONS KW - and KW - bands KW - ism KW - lines KW - molecules AU - Motylewski, T AU - Linnartz, H AU - Vaizert, O AU - Maier, JP AU - Galazutdinov, GA AU - Musaev, FA AU - Krebowski, J AU - Walker, GAH AU - Bohlender, DA PY - 2000/// UR - http://www.iop.org/EJ/article/0004-637X/531/1/312/50370.web.pdf?request-id=e0cead8e-2f13-45ec-8329-7f3d297b8c88 ER -