University of Hertfordshire

From the same journal

A Large Scale, Low Frequency Murchison Widefield Array Survey of Galactic HII regions between 260\340

Research output: Contribution to journalArticlepeer-review


  • L. Hindson
  • M. Johnston-Hollitt
  • N. Hurley-Walker
  • J. R. Callingham
  • H. Su
  • J. Morgan
  • M. Bell
  • G. Bernardi
  • J. D. Bowman
  • F. Briggs
  • R. J. Cappallo
  • A. A. Deshpande
  • K. S. Dwarakanath
  • B. -Q For
  • B. M. Gaensler
  • L. J. Greenhill
  • P. Hancock
  • B. J. Hazelton
  • A. D. Kapinska
  • D. L. Kaplan
  • And 23 others
  • E. Lenc
  • C. J. Lonsdale
  • B. Mckinley
  • S. R. McWhirter
  • D. A. Mitchell
  • M. F. Morales
  • E. Morgan
  • D. Oberoi
  • A. Offringa
  • S. M. Ord
  • P. Procopio
  • T. Prabu
  • N. UdayaShankar
  • K. S. Srivani
  • L. Staveley-Smith
  • R. Subrahmanyan
  • S. J. Tingay
  • R. B. Wayth
  • R. L. Webster
  • A. Williams
  • C. L. Williams
  • C. Wu
  • Q. Zheng
View graph of relations
Original languageEnglish
Article numbere020
JournalPublications of the Astronomical Society of Australia
Publication statusPublished - 17 May 2016


We have compiled a catalogue of HII regions detected with the Murchison Widefield Array (MWA) between 72 and 231MHz. The multiple frequency bands provided by the MWA allow us identify the characteristic spectrum generated by the thermal Bremsstrahlung process in HII regions. We detect 302 HII regions between 260


Publications of the Astronomical Society of Australia (PASA), Vol. 33, e020, 17 pages (2016). © Astronomical Society of Australia 2016; published by Cambridge University Press. The online version of this article is published within an Open Access environment subject to the conditions of the Creative Commons Attribution-NonCommercial-ShareAlike license by-nc-sa/3.0/. The written permission of Cambridge University Press must be obtained for commercial re-use. doi:10.1017/pasa.2016.19


ID: 10291435