Brett A. McGuire

Carma observations of L1157: chemical complexity in the shocked outflow

ANDREW M BURKHARDT, NIKLAUS M DOLLHOPF, JOANNA F. CORBY, Department of Astronomy, The University of Virginia, Charlottesville, VA, USA; BRANDON CARROLL, Division of Chemistry and Chemical Engineering, California Institute of Technology, Pasadena, CA, USA; CHRISTOPHER N SHINGLEDECKER, Department of Chemistry, The University of Virginia, Charlottesville, VA, USA; RYAN LOOMIS, Department of Astronomy, Harvard University, Cambridge, MA, USA; S. TOM BOOTH, Department of Astronomy, The University of Virginia, Charlottesville, VA, USA; GEOFFREY BLAKE, Division of Chemistry and Chemical Engineering, California Institute of Technology, Pasadena, CA, USA; ANTHONY REMIJAN, ALMA, National Radio Astronomy Observatory, Charlottesville, VA, USA; BRETT A. McGUIRE, NAASC, National Radio Astronomy Observatory, Charlottesville, VA, USA.

THE CURIOUS CASE OF NH2OH: HUNTING A DIRECT AMINO ACID PRECURSOR SPECIES IN THE INTERSTELLAR MEDIUM

BRETT A. McGUIRE, NAASC, National Radio Astronomy Observatory, Charlottesville, VA, USA; BRANDON CARROLL, Division of Chemistry and Chemical Engineering, California Institute of Technology, Pasadena, CA, USA; NIKLAUS M DOLLHOPF, Department of Astronomy, The University of Virginia, Charlottesville, VA, USA; NATHAN CROCKETT, Geological and Planetary Sciences , California Institute of Techonolgy, Pasadena, CA, USA; GEOFFREY BLAKE, Division of Chemistry and Chemical Engineering, California Institute of Technology, Pasadena, CA, USA; ANTHONY REMIJAN, ALMA, National Radio Astronomy Observatory, Charlottesville, VA, USA.

THz Time-domain spectroscopy of complex interstellar ice analogs

SERGIO IOPPOLO, Geological and Planetary Sciences , California Institute of Techonolgy, Pasadena, CA, USA; BRETT A. McGUIRE, MARCO A. ALLODI, Division of Chemistry and Chemical Engineering, California Institute of Technology, Pasadena, CA, USA; XANDER DE VRIES, Theoretical Chemistry, University of Nijmegen, Nijmegen, Netherlands; IAN FINNERAN, BRANDON CARROLL, GEOFFREY BLAKE, Division of Chemistry and Chemical Engineering, California Institute of Technology, Pasadena, CA, USA.

TIME-DOMAIN TERAHERTZ SPECTRSOCOPY OF POLYCYCLIC AROMATIC HYDROCARBONS

Polycyclic arom. hydrocarbons (PAHs) are believed to be the carriers of the unidentified IR features (UIRs), and as such may account for up to 20 of the interstellar carbon budget. In addn., PAHs may play a significant role in carbon grain formation, and affect many chem. and phys. processes in the interstellar medium. However, it is difficult to distinguish individual PAHs in the near- to mid-IR region of the spectrum, and our failure to unambiguously detect PAHs hinders our ability to evaluate the role they play. One possible soln. is observations in the TeraHertz (THz) (or far-IR, from 0.1 to 10 THz or 3 to 330 cm^(-1)) regime. Recent work in the THz region of the electromagnetic spectrum has shown that the identity of complex mol. solids can be detd. from their THz spectra, and the time-domain THz spectrometer developed in our lab. has the ability to measure the full complex index of refraction in a single measurement, thus aiding in the identification of complex solids. In addn., recent advances in THz technol. have enabled both lab. spectroscopy and astronomical observations in this region. A first step in both lab. and astronomical studies of PAHs is the acquisition of spectra of pure PAH samples. We present the THz time-domain spectra (0.5 - 7 THz) of several PAHs, including naphthalene, anthracene, and pyrene, and discuss the utility of these spectra for future lab. and astronomical studies.