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Displaying 51 - 75 of 320

Confirmation of Interstellar Methycyanodiacetylene (CH3C5N)

April 11, 2006
Author(s)
Lewis E. Snyder, J M. Hollis, P R. Jewell, Francis J. Lovas, A J. Remijan
Ten spectral lines of the symmetric-top molecule methylcyanodiacetylene (CH3C5N) have been detected with the 100 m Green Bank Telescope (GBT) toward the Taurus molecular cloud TMC-1. Both K=0 and K=1 components of the 12K-11K, 13K-12K, 14K-13K, 15K-14K

Hyperfine Structure Identification of Interstellar Cyanoallene Toward TMC-1

January 10, 2006
Author(s)
Francis J. Lovas, A Remijan, J M. Hollis, P R. Jewell, Lewis E. Snyder
Interstellar cyanoallene (CH2CCHCN) has been detected with the 100-m Green Bank Telescope (GBT) toward the dark Taurus Molecular Cloud (TMC-1) by means of the 414-313, 404-303, 515 -414, and 505-404 rotational transitions at 20.2 GHz, 20.6 GHz, 25.2 GHz

Microwave Spectrum and Structure of Methyl Phosphonic Difluoride

January 2, 2006
Author(s)
R D. Suenram, Francis J. Lovas, David F. Plusquellic, M W. Elizy, J M. Lochner, J O. Jensen, A C. Samuels
The rotational spectrum of methyl phosphonic difluoride has been reinvestigated using a pulsed-molecular-beam Fabry-Perot cavity microwave spectrometer. The enhanced resolution of the Fourier transform microwave (FTMW) spectrometer (compared to the

Interstellar Isomers: The Importance of Bonding Energy Differences

October 10, 2005
Author(s)
A J. Remijan, J M. Hollis, Francis J. Lovas, David F. Plusquellic, P R. Jewell
We present new observations of large cyanide molecules and their corresponding isocyanide isomers toward the Sgr B2(N)molecular cloud. We report the first detection of the JK=10-00 transition of methyl isocyanide (CH3NC) with the 100-m Green Bank Telescope

Interstellar Chemistry: A Strategy for Detecting Polycyclic Aromatic Hydrocarbons in Space

March 1, 2005
Author(s)
Francis J. Lovas, R J. McMahon, J-U Grabow, M Schnell, J Mack, L T. Scott, R L. Kuczkowski
Polycyclic aromatic hydrocarbons (PAHs) represent important targets for radio astronomy because they offer the possibilities of validating the PAH hypothesis and revealing new insight into the chemistry of interstellar space. Polycyclic aromatic