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Results: 1-9 |
Results: 9
Radiative electron attachment to small linear carbon clusters and its significance for the chemistry of diffuse interstellar clouds
Authors: Terzieva, R Herbst, E
Citation: R. Terzieva et E. Herbst, Radiative electron attachment to small linear carbon clusters and its significance for the chemistry of diffuse interstellar clouds, INT J MASS, 201(1-3), 2000, pp. 135-142
The physics and chemistry of small translucent molecular clouds. XIII. Thebasic hydrocarbon chemistry
Authors: Turner, BE Herbst, E Terzieva, R
Citation: Be. Turner et al., The physics and chemistry of small translucent molecular clouds. XIII. Thebasic hydrocarbon chemistry, ASTROPH J S, 126(2), 2000, pp. 427-460
The possibility of nitrogen isotopic fractionation in interstellar clouds
Authors: Terzieva, R Herbst, E
Citation: R. Terzieva et E. Herbst, The possibility of nitrogen isotopic fractionation in interstellar clouds, M NOT R AST, 317(3), 2000, pp. 563-568
Calculations on the rates, mechanisms, and interstellar importance of the reactions between C and NH2 and between N and CH2
Authors: Herbst, E Terzieva, R Talbi, D
Citation: E. Herbst et al., Calculations on the rates, mechanisms, and interstellar importance of the reactions between C and NH2 and between N and CH2, M NOT R AST, 311(4), 2000, pp. 869-876
The abundance of C((7))over-bar in diffuse clouds
Authors: Ruffle, DP Bettens, RPA Terzieva, R Herbst, E
Citation: Dp. Ruffle et al., The abundance of C((7))over-bar in diffuse clouds, ASTROPHYS J, 523(2), 1999, pp. 678-682
A molecular orbital study of the HC3NH+ + e(-) dissociative recombination and its role in the production of cyanoacetylene isomers in interstellar clouds
Authors: Osamura, Y Fukuzawa, K Terzieva, R Herbst, E
Citation: Y. Osamura et al., A molecular orbital study of the HC3NH+ + e(-) dissociative recombination and its role in the production of cyanoacetylene isomers in interstellar clouds, ASTROPHYS J, 519(2), 1999, pp. 697-704
The physics and chemistry of small translucent molecular clouds. XII. Morecomplex species explainable by gas-phase processes
Authors: Turner, BE Terzieva, R Herbst, E
Citation: Be. Turner et al., The physics and chemistry of small translucent molecular clouds. XII. Morecomplex species explainable by gas-phase processes, ASTROPHYS J, 518(2), 1999, pp. 699-732
New H and H-2 reactions with small hydrocarbon ions and their roles in benzene synthesis in dense interstellar clouds
Authors: McEwan, MJ Scott, GBI Adams, NG Babcock, LM Terzieva, R Herbst, E
Citation: Mj. Mcewan et al., New H and H-2 reactions with small hydrocarbon ions and their roles in benzene synthesis in dense interstellar clouds, ASTROPHYS J, 513(1), 1999, pp. 287-293
The sensitivity of gas-phase chemical models of interstellar clouds to C and O elemental abundances and to a new formation mechanism for ammonia (vol501, pg 207, 1998)
Authors: Terzieva, R Herbst, E
Citation: R. Terzieva et E. Herbst, The sensitivity of gas-phase chemical models of interstellar clouds to C and O elemental abundances and to a new formation mechanism for ammonia (vol501, pg 207, 1998), ASTROPHYS J, 509(2), 1998, pp. 932-932
Risultati: 1-9 |