Molecular abundances in IRC + 10216

[1]  D. Spears,et al.  The brightness distribution of IRC +10216 at 11 microns , 1979 .

[2]  P. J. Huggins,et al.  High-resolution observations of CO in IRC + 10216 and three related objects , 1979 .

[3]  M. Cohen.  Circumstellar envelopes and the evolution of carbon stars. , 1979 .

[4]  D. Spears,et al.  NH3 in IRC +10216 , 1979 .

[5]  M. Reid,et al.  Molecular emission from expanding envelopes around evolved stars. II - SiO - On the mechanism of mass loss and the efficiency of grain formation , 1979 .

[6]  P. Martin,et al.  Circumstellar dust envelopes: calculation of eclipse light curves and fringe visibilities. , 1979 .

[7]  N. Evans,et al.  Molecular abundance variations in interstellar clouds. , 1978 .

[8]  M. Allen,et al.  Radio observations of interstellar CN toward diffuse clouds, dark clouds, black clouds, and circumstellar clouds , 1978 .

[9]  R. Linke,et al.  Isotope abundance anomalies in IRC +10216 , 1978 .

[10]  J. D. Fix,et al.  Models of mass flows from cool, luminous stars , 1978 .

[11]  P. Thaddeus,et al.  Detection of the C4H radical toward IRC plus 10216 , 1978 .

[12]  E. Iglesias.  The chemical evolution of molecular clouds , 1977 .

[13]  R. Clegg,et al.  Molecular spectra of pure S stars , 1977 .

[14]  F. Hill,et al.  The circumstellar envelope of IRC +10216 , 1977 .

[15]  R. Kakar,et al.  Unidentified lines in molecular clouds and a search for C-14 in IRC +10216 , 1977 .

[16]  P. Thaddeus,et al.  Tentative detection of the C/sub 3/N radical , 1977 .

[17]  S. Ridgway,et al.  Circumstellar methane in the infrared spectrum of IRC+10°216 , 1976, Nature.

[18]  L. Willson.  Shock-wave interpretation of emission lines in long-period variable stars. I. The velocity of the shock. , 1976 .

[19]  L. Lucy.  Mass Loss by Cool Carbon Stars , 1976 .

[20]  G. Knapp,et al.  CO observations of the expanding envelope of IRC +10216. , 1976 .

[21]  B. Turner,et al.  Interstellar CN at radio wavelengths. , 1975 .

[22]  M. Morris.  The IRC+10216 molecular envelope , 1975 .

[23]  R. C. Gilman.  Planck Mean Cross-Sections for Four Grain Materials , 1974 .

[24]  P. Thaddeus,et al.  The ethynyl radical C2H - A new interstellar molecule , 1974 .

[25]  E. Anders,et al.  Interstellar Molecules: Origin by Catalytic Reactions on Grain Surfaces? , 1974 .

[26]  P. K. Pearson,et al.  Some properties of H$sub 2$CN$sup +$: A potentially important interstellar species , 1974 .

[27]  R. Treffers,et al.  High-resolution spectra of cool stars in the 10- and 20-micron regions , 1974 .

[28]  T. Geballe,et al.  Observations of carbon monoxide at 4.7 microns in IRC + 10216, VY Canis Majoris, and NML Cygni. , 1973 .

[29]  W. Wilson,et al.  Carbon monoxide and hydrogen cyanide millimeter-wave emission from stars , 1973 .

[30]  E. Becklin,et al.  Infrared diameter of IRC + 10216 determined from lunar occultations. , 1972 .

[31]  G. Herbig,et al.  Near-Infrared Spectra of NML Cygnt and IRC+10216 , 1970 .

[32]  R. C. Gilman.  On the composition of circumstellar grains. , 1969 .

[33]  G. Wallersteín.  The Physical Properties of Carbon Stars , 1973 .

[34]  W. D. Watson,et al.  MOLECULE FORMATION ON INTERSTELLAR GRAINS. , 1972 .

[35]  B. Zuckerman,et al.  HCN IN IRC + 10216. , 1971 .

[36]  R. Wilson,et al.  Millimeter Observations of co, cn, and CS Emission from IRC+10216 , 1971 .

[37]  R. Wilson,et al.  Observation of CO emission at 2.6 millimeters from IRC plus 10216 , 1971 .

[38]  G. Lockwood.  NEAR-INFRARED PHOTOMETRY OF TWO EXTREMELY RED OBJECTS. , 1970 .

[39]  Joseph S. Miller.  SCANNER OBSERVATIONS OF THE LEO INFRARED OBJECT IRC + 10216. , 1970 .

[40]  G. Neugebauer,et al.  The Unusual Infrared Object IRC+10216 , 1969 .