A First Look for Molecules between 103 and 133 MHz using the Murchison Widefield Array
arXiv:1707.06009 · doi:10.1093/mnras/stx1838
Abstract
We detail and present results from a pilot study to assess the feasibility of detecting molecular lines at low radio frequencies. We observed a 400 square degree region centred on the Galactic Centre with the Murchison Widefield Array (MWA) between 103 and 133\,MHz targeting 28 known molecular species that have significant transitions. The results of this survey yield tentative detections of nitric oxide (NO) and the mercapto radical (SH). Both of these molecules appear to be associated with evolved stars.
Accepted MNRAS, 13 pages, 6 figures, 3 Tables
References in corpus (12)
- WSClean: an implementation of a fast, generic wide-field imager for radio astronomy
- GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey I: A low-frequency extragalactic catalogue
- Discovery of the Interstellar Chiral Molecule Propylene Oxide (CHCHCHO)
- Post-correlation radio frequency interference classification methods
- The low-frequency environment of the Murchison Widefield Array: radio-frequency interference analysis and mitigation
- A Search for Propylene Oxide and Glycine in Sagittarius B2 (LMH) and Orion
- The Murchison Widefield Array Commissioning Survey: A Low-Frequency Catalogue of 14,110 Compact Radio Sources over 6,100 Square Degrees
- Search for Interstellar monohydric Thiols
- Herschel HIFI observations of O toward Orion: special conditions for shock enhanced emission
- MALT-45: A 7 mm survey of the southern Galaxy - I. Techniques and spectral line data
- A Digital-Receiver for the Murchison Widefield Array
- A Large Scale, Low Frequency Murchison Widefield Array Survey of Galactic HII regions between 260< l <\340
Cited by in corpus (4)
- Science with the Murchison Widefield Array: Phase I Results and Phase II Opportunities
- A SETI Survey of the Vela Region using the Murchison Widefield Array: Orders of Magnitude Expansion in Search Space
- Spectroscopy with the Engineering Development Array: cold H at 63 MHz towards the Galactic Centre
- First Search for Low-Frequency CH with a Square Kilometre Array Precursor Telescope