Searcharxiv⌕ Search

arXiv subjects

Brett A. McGuire

Publications and source records attributed to Brett A. McGuire.

93 records · Page 6Linked to original sources

A CSO Broadband Spectral Line Survey of Sgr B2(N)-LMH from 260 - 286 GHz

Presented here are the results of a broadband spectral line survey of the Sgr B2(N) - LMH region from 260 - 286 GHz using the Caltech Submillimeter Observatory. The data were taken over the course of a single night (May 26, 2013) during the course of science testing of the remote observational capabilities of the facility. The data are freely available to public both as raw, double-side band observational data and as a minimally-reduced ascii spectrum. The procedural scripts used for the preliminary data reduction using CLASS are provided as well. The observational parameters and preliminary data reduction procedures are detailed. Finally, we provide instructions for accessing the data as well as comment on the robustness of the preliminary reduction.

astro-ph.GA↗

Interstellar Carbodiimide (HNCNH) - A New Astronomical Detection from the GBT PRIMOS Survey via Maser Emission Features

In this work, we identify carbodiimide (HNCNH), which is an isomer of the well-known interstellar species cyanamide (NH2CN), in weak maser emission, using data from the GBT PRIMOS survey toward Sgr B2(N). All spectral lines observed are in emission and have energy levels in excess of 170 K, indicating that the molecule likely resides in relatively hot gas that characterizes the denser regions of this star forming region. The anticipated abundance of this molecule from ice mantle experiments is ~10% of the abundance of NH2CN, which in Sgr B2(N) corresponds to ~2 x 10^13 cm-2. Such an abundance results in transition intensities well below the detection limit of any current astronomical facility and, as such, HNCNH could only be detected by those transitions which are amplified by masing.

astro-ph.GA↗

A Search for Hydroxylamine (NH2OH) toward Select Astronomical Sources

Observations of 14 rotational transitions of hydroxylamine (NH2OH) using the NRAO 12 m Telescope on Kitt Peak are reported towards IRC+10216, Orion KL, Orion S, Sgr B2(N), Sgr B2(OH), W3IRS5, and W51M. Although recent models suggest the presence of NH2OH in high abundance, these observations resulted in non-detection. Upper limits are calculated to be as much as six orders of magnitude lower than predicted by models. Possible explanations for the lower than expected abundance are explored.

astro-ph.GA↗