A Large Scale, Low Frequency Murchison Widefield Array Survey of Galactic HII regions between 260\340
Hindson, L., Johnston-Hollitt, M., Hurley-Walker, N., Callingham, J. R., Su, H., Morgan, J., Bell, M., Bernardi, G., Bowman, J. D., Briggs, F., Cappallo, R. J., Deshpande, A. A., Dwarakanath, K. S., For, B. -Q, Gaensler, B. M., Greenhill, L. J., Hancock, P., Hazelton, B. J., Kapinska, A. D., Kaplan, D. L., Lenc, E., Lonsdale, C. J., Mckinley, B., McWhirter, S. R., Mitchell, D. A., Morales, M. F., Morgan, E., Oberoi, D., Offringa, A., Ord, S. M., Procopio, P., Prabu, T., UdayaShankar, N., Srivani, K. S., Staveley-Smith, L., Subrahmanyan, R., Tingay, S. J., Wayth, R. B., Webster, R. L., Williams, A., Williams, C. L., Wu, C. and Zheng, Q.
(2016)
A Large Scale, Low Frequency Murchison Widefield Array Survey of Galactic HII regions between 260\340.
Publications of the Astronomical Society of Australia, 33: e020.
ISSN 1323-3580
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
Item Type | Article |
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Additional information | 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 http://creativecommons.org/licenses/ 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 |
Keywords | astro-ph.ga |
Date Deposited | 15 May 2025 13:10 |
Last Modified | 31 May 2025 00:05 |