These tools will no longer be maintained as of December 31, 2024. Archived website can be found here. PubMed4Hh GitHub repository can be found here. Contact NLM Customer Service if you have questions.


Pubmed for Handhelds

PUBMED FOR HANDHELDS

Journal Abstract Search

409 related items for PubMed ID: 11538104

  • 1. Laboratory studies of the newly discovered infrared band at 4705.2 cm-1 (2.1253 micrometers) in the spectrum of Io: the tentative identification of CO2.
    Sandford SA, Salama F, Allamandola LJ, Trafton LM, Lester DF, Ramseyer TF.
    Icarus; 1991; 91():125-44. PubMed ID: 11538104
    [Abstract] [Full Text] [Related]

  • 2. The 2.5-5.0 micrometers spectra of Io: evidence for H2S and H2O frozen in SO2.
    Salama F, Allamandola LJ, Witteborn FC, Cruikshank DP, Sandford SA, Bregman JD.
    Icarus; 1990 Jan; 83(1):66-82. PubMed ID: 11538411
    [Abstract] [Full Text] [Related]

  • 3. A new class of absorption feature in Io's near-infrared spectrum.
    Trafton LM, Lester DF, Ramseyer TF, Salama F, Sandford SA, Allamandola LJ.
    Icarus; 1991 Jan; 89():264-76. PubMed ID: 11538100
    [Abstract] [Full Text] [Related]

  • 4. The physical and infrared spectral properties of CO2 in astrophysical ice analogs.
    Sandford SA, Allamandola LJ.
    Astrophys J; 1990 May 20; 355(1):357-72. PubMed ID: 11538691
    [Abstract] [Full Text] [Related]

  • 5. Is H2O present on Io? The detection of a new strong band near 3590 cm-1 (2.79 micrometers).
    Salama F, Allamandola LJ, Sandford SA, Bregman JD, Witteborn FC, Cruikshank DP.
    Icarus; 1994 May 20; 107():413-7. PubMed ID: 11539181
    [Abstract] [Full Text] [Related]

  • 6.
    ; . PubMed ID:
    [No Abstract] [Full Text] [Related]

  • 7. Interstellar solid CO: polar and nonpolar interstellar ices.
    Tielens AG, Tokunaga AT, Geballe TR, Baas F.
    Astrophys J; 1991 Nov 01; 381(1 Pt 1):181-99. PubMed ID: 11538393
    [Abstract] [Full Text] [Related]

  • 8.
    ; . PubMed ID:
    [No Abstract] [Full Text] [Related]

  • 9.
    ; . PubMed ID:
    [No Abstract] [Full Text] [Related]

  • 10. Infrared spectroscopy of dense clouds in the C-H stretch region: methanol and "diamonds.".
    Allamandola LJ, Sandford SA, Tielens AG, Herbst TM.
    Astrophys J; 1992 Nov 01; 399():134-46. PubMed ID: 11540063
    [Abstract] [Full Text] [Related]

  • 11. The 2140 cm-1 (4.673 microns) solid CO band: the case for interstellar O2 and N2 and the photochemistry of nonpolar interstellar ice analogs.
    Elsila J, Allamandola LJ, Sandford SA.
    Astrophys J; 1997 Apr 20; 479(2 Pt 1):818-38. PubMed ID: 11540158
    [Abstract] [Full Text] [Related]

  • 12. Infrared spectroscopy of Triton and Pluto ice analogs: the case for saturated hydrocarbons.
    Bohn RB, Sandford SA, Allamandola LJ, Cruikshank DP.
    Icarus; 1994 Sep 20; 111(1):151-73. PubMed ID: 11539177
    [Abstract] [Full Text] [Related]

  • 13. Unraveling the 10 micron "silicate" feature of protostars: the detection of frozen interstellar ammonia.
    Lacy JH, Faraji H, Sandford SA, Allamandola LJ.
    Astrophys J; 1998 Jul 01; 501(1 Pt 2):L105-9. PubMed ID: 11542938
    [Abstract] [Full Text] [Related]

  • 14. Interstellar polycyclic aromatic hydrocarbons: the infrared emission bands, the excitation/emission mechanism, and the astrophysical implications.
    Allamandola LJ, Tielens AG, Barker JR.
    Astrophys J Suppl Ser; 1989 Dec 01; 71():733-75. PubMed ID: 11542189
    [Abstract] [Full Text] [Related]

  • 15.
    ; . PubMed ID:
    [No Abstract] [Full Text] [Related]

  • 16.
    ; . PubMed ID:
    [No Abstract] [Full Text] [Related]

  • 17. Condensation and vaporization studies of CH3OH and NH3 ices: major implications for astrochemistry.
    Sandford SA, Allamandola LJ.
    Astrophys J; 1993 Nov 10; 417(2):815-25. PubMed ID: 11540092
    [Abstract] [Full Text] [Related]

  • 18.
    ; . PubMed ID:
    [No Abstract] [Full Text] [Related]

  • 19.
    ; . PubMed ID:
    [No Abstract] [Full Text] [Related]

  • 20.
    ; . PubMed ID:
    [No Abstract] [Full Text] [Related]

    Page: [Next] [New Search]
    of 21.