Search Results - "Schieven, G. H"

Refine Results
  1. 1

    A measurement of the 362 GHz absorption line of Mars atmospheric H2O2 by CLANCY, R. T, SANDOR, B. J, MORIARTY-SCHIEVEN, G. H

    Published in Icarus (New York, N.Y. 1962) (01-03-2004)
    “…The 362.156 GHz absorption spectrum of H2O2 in the Mars atmosphere was observed on September 4 of 2003, employing the James Clerk Maxwell Telescope (JCMT)…”
    Get full text
    Journal Article
  2. 2
  3. 3
  4. 4
  5. 5
  6. 6
  7. 7
  8. 8
  9. 9

    Observational definition of the Venus mesopause: vertical structure, diurnal variation, and temporal instability by Clancy, R.T., Sandor, B.J., Moriarty-Schieven, G.H.

    Published in Icarus (New York, N.Y. 1962) (2003)
    “…Submillimeter line observations of CO in the Venus middle atmosphere (mesosphere) were observed with the James Clerk Maxwell Telescope (JCMT, Mauna Kea) about…”
    Get full text
    Journal Article
  10. 10
  11. 11
  12. 12
  13. 13

    Venus upper atmospheric CO, temperature, and winds across the afternoon/evening terminator from June 2007 JCMT sub-millimeter line observations by Clancy, R.T., Sandor, B.J., Moriarty-Schieven, G.H.

    Published in Planetary and space science (01-08-2008)
    “…The Venus mesosphere constitutes a highly variable transition region between the zonal rotation of the lower atmosphere and the diurnal circulation of the…”
    Get full text
    Journal Article
  14. 14
  15. 15

    First observation of CO at 345 GHz in the atmosphere of Saturn with the JCMT: New constraints on its origin by Cavalié, T., Billebaud, F., Dobrijevic, M., Fouchet, T., Lellouch, E., Encrenaz, T., Brillet, J., Moriarty-Schieven, G.H., Wouterloot, J.G.A., Hartogh, P.

    Published in Icarus (New York, N.Y. 1962) (2009)
    “…We have performed the first observation of the CO(3-2) spectral line in the atmosphere of Saturn with the James Clerk Maxwell Telescope. We have used a…”
    Get full text
    Journal Article
  16. 16

    The L1457 Molecular/Atomic Cloud Complex: H I and CO Maps by Moriarty-Schieven, G. H, Wannier, and P. G

    Published in The Astrophysical journal (01-02-1997)
    “…L1457 is the closest known molecular cloud (65 pc), and it lies near the edge of the local hot bubble and well out of the Galactic plane (b approximately -34…”
    Get full text
    Journal Article
  17. 17

    L1551NE—Discovery of a Binary Companion by Moriarty-Schieven, G. H, Powers, J. A, Butner, H. M, Wannier, P. G, Keene, Jocelyn

    Published in The Astrophysical journal (20-04-2000)
    “…L1551NE is a very young (class 0 or I) low-mass protostar located close to the well-studied L1551 IRS 5. Here we present evidence, from 1.3 mm continuum…”
    Get full text
    Journal Article
  18. 18
  19. 19

    A High-Resolution Map of (12)CO J= 6-5 Emission in the Starburst Galaxy M82 by Seaquist, E R, Lee, S W, Moriarty-Schieven, G H

    Published in The Astrophysical journal (10-02-2006)
    “…We present a map of (12)CO J = 6-5 emission of the nuclear region of the nearby starburst galaxy M82 at resolution 7" taken with the James Clerk Maxwell…”
    Get full text
    Journal Article
  20. 20

    High-resolution images of the L1551 bipolar outflow: evidence for an expanding, accelerated shell by Moriarty-Schieven, G H, Snell, R L, Strom, S E, Schloerb, F P, Strom, K M

    Published in The Astrophysical journal (15-08-1987)
    “…Approximately one-half of the L1551 bipolar outflow was mapped in the J = 1-0 transition of 12CO using the FCRAO 14 m telescope. The data were obtained by…”
    Get more information
    Journal Article