Hydrogenation of Interstellar Molecules: A Survey for Methylenimine (CH2NH)
暂无分享,去创建一个
[1] T. Millar,et al. A 330-360 GHz spectral survey of G 34.3+0.15. I. Data and physical analysis , 1996 .
[2] E. Herbst,et al. Fractional abundances of molecules in dense interstellar clouds: A compendium of recent model results. , 1996 .
[3] Scott A. Sandford,et al. Organic Compounds Produced by Photolysis of Realistic Interstellar and Cometary Ice Analogs Containing Methanol , 1995 .
[4] W. Danchi,et al. The distribution of molecules in the core of OMC-1 , 1995 .
[5] J. Watson,et al. A spectral-line survey of W51 from 17.6 to 22.0 GHz , 1993 .
[6] A. Marscher,et al. Detection of AU-Scale Structure in Molecular Clouds , 1993 .
[7] B. Turner. A Molecular Line Survey of Sagittarius B2 and Orion--KL from 70 to 115 GHz. II. Analysis of the Data , 1991 .
[8] W. Irvine,et al. Chemical abundances in cold, dark interstellar clouds. , 1991, Icarus.
[9] W. Welch,et al. Dynamical collapse of the W51 star-forming region , 1990 .
[10] J. Stutzki,et al. Strong, spatially extended CO 7-6 emission from luminous cloud cores - W51 and DR 21 , 1989 .
[11] R. Genzel,et al. Warm dense gas in luminous protostellar regions - a submillimeter and far-infrared CO line study , 1987 .
[12] Geoffrey A. Blake,et al. Molecular abundances in OMC-1 - the chemical composition of interstellar molecular clouds and the influence of massive star formation , 1987 .
[13] M. Joy,et al. High angular resolution infrared mapping of the compact H II regions W51 and DR 21/W75 , 1986 .
[14] E. Becklin,et al. The massive core of W51 , 1984 .
[15] E. Herbst,et al. Laboratory measurements of ion-molecule reactions pertaining to interstellar hydrocarbon synthesis , 1983 .
[16] P. Ho. VLA observations of warm NH/sub 3/ associated with mass outflows in W51 , 1983 .
[17] P. Goldsmith,et al. DETERMINATION OF THE HNC TO HCN ABUNDANCE RATIO IN GIANT MOLECULAR CLOUDS , 1981 .
[18] J. Dickerson. Stability of nonautonomous second-order partial differential equations , 1978 .
[19] P. Thaddeus,et al. On the relationship of interstellar N2H/+/, HCO/+/, HCN, and CN , 1977 .
[20] N. Kaifu,et al. Detection of Interstellar Methylamine , 1974 .
[21] W. Irvine,et al. The chemical composition of interstellar molecular clouds , 2004, Origins of life.
[22] W. Irvine,et al. Molecular Abundance Variations Among and Within Cold, Dark Molecular Clouds , 1992 .
[23] W. Irvine,et al. Upper limits for the ethyl-cyanide abundances in TMC-1 and L134N: Chemical implications , 1991, Astrophysics and space science.
[24] J. Bieging. The W 51 source complex , 1975 .
[25] F. Lovas,et al. Microwave Spectra of Molecules of Astrophysical Interest: II Methylenimine , 1973 .