A first look for molecules between 103 and 133MHz using the Murchison Widefield Array

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 speci...

Full description

Bibliographic Details
Main Authors: Tremblay, C., Hurley-Walker, N., Cunningham, M., Jones, P., Hancock, Paul, Wayth, R., Jordan, C.
Format: Journal Article
Published: Oxford University Press 2017
Online Access:http://hdl.handle.net/20.500.11937/57960
http://dx.doi.org/10.1093/mnras/stx1838
_version_ 1848760142953185280
author Tremblay, C.
Hurley-Walker, N.
Cunningham, M.
Jones, P.
Hancock, Paul
Wayth, R.
Jordan, C.
author_facet Tremblay, C.
Hurley-Walker, N.
Cunningham, M.
Jones, P.
Hancock, Paul
Wayth, R.
Jordan, C.
author_sort Tremblay, C.
building Curtin Institutional Repository
collection Online Access
description 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.
first_indexed 2025-11-14T10:11:05Z
format Journal Article
id curtin-20.500.11937-57960
institution Curtin University Malaysia
institution_category Local University
last_indexed 2025-11-14T10:11:05Z
publishDate 2017
publisher Oxford University Press
recordtype eprints
repository_type Digital Repository
spelling curtin-20.500.11937-579602019-02-19T05:36:14Z A first look for molecules between 103 and 133MHz using the Murchison Widefield Array Tremblay, C. Hurley-Walker, N. Cunningham, M. Jones, P. Hancock, Paul Wayth, R. Jordan, C. 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. 2017 Journal Article http://hdl.handle.net/20.500.11937/57960 10.1093/mnras/stx1838 http://dx.doi.org/10.1093/mnras/stx1838 Oxford University Press restricted
spellingShingle Tremblay, C.
Hurley-Walker, N.
Cunningham, M.
Jones, P.
Hancock, Paul
Wayth, R.
Jordan, C.
A first look for molecules between 103 and 133MHz using the Murchison Widefield Array
title A first look for molecules between 103 and 133MHz using the Murchison Widefield Array
title_full A first look for molecules between 103 and 133MHz using the Murchison Widefield Array
title_fullStr A first look for molecules between 103 and 133MHz using the Murchison Widefield Array
title_full_unstemmed A first look for molecules between 103 and 133MHz using the Murchison Widefield Array
title_short A first look for molecules between 103 and 133MHz using the Murchison Widefield Array
title_sort first look for molecules between 103 and 133mhz using the murchison widefield array
url http://hdl.handle.net/20.500.11937/57960
http://dx.doi.org/10.1093/mnras/stx1838