Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/26319
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Hindson, L. | en_US |
dc.contributor.author | Johnston-Hollitt, M. | en_US |
dc.contributor.author | Hurley-Walker, N. | en_US |
dc.contributor.author | Callingham, J. R. | en_US |
dc.contributor.author | Su, H. | en_US |
dc.contributor.author | Morgan, J. | en_US |
dc.contributor.author | Bell, M. | en_US |
dc.contributor.author | BERNARDI, GIANNI | en_US |
dc.contributor.author | Bowman, J. D. | en_US |
dc.contributor.author | Briggs, F. | en_US |
dc.contributor.author | Cappallo, R. J. | en_US |
dc.contributor.author | Deshpande, A. A. | en_US |
dc.contributor.author | Dwarakanath, K. S. | en_US |
dc.contributor.author | For, B. -Q. | en_US |
dc.contributor.author | Gaensler, B. M. | en_US |
dc.contributor.author | Greenhill, L. J. | en_US |
dc.contributor.author | Hancock, P. | en_US |
dc.contributor.author | Hazelton, B. J. | en_US |
dc.contributor.author | Kapińska, A. D. | en_US |
dc.contributor.author | Kaplan, D. L. | en_US |
dc.contributor.author | Lenc, E. | en_US |
dc.contributor.author | Lonsdale, C. J. | en_US |
dc.contributor.author | Mckinley, B. | en_US |
dc.contributor.author | McWhirter, S. R. | en_US |
dc.contributor.author | Mitchell, D. A. | en_US |
dc.contributor.author | Morales, M. F. | en_US |
dc.contributor.author | Morgan, E. | en_US |
dc.contributor.author | Oberoi, D. | en_US |
dc.contributor.author | Offringa, A. | en_US |
dc.contributor.author | Ord, S. M. | en_US |
dc.contributor.author | Procopio, P. | en_US |
dc.contributor.author | Prabu, T. | en_US |
dc.contributor.author | Shankar, N. Udaya | en_US |
dc.contributor.author | Srivani, K. S. | en_US |
dc.contributor.author | Staveley-Smith, L. | en_US |
dc.contributor.author | Subrahmanyan, R. | en_US |
dc.contributor.author | Tingay, S. J. | en_US |
dc.contributor.author | Wayth, R. B. | en_US |
dc.contributor.author | Webster, R. L. | en_US |
dc.contributor.author | Williams, A. | en_US |
dc.contributor.author | Williams, C. L. | en_US |
dc.contributor.author | Wu, C. | en_US |
dc.contributor.author | Zheng, Q. | en_US |
dc.date.accessioned | 2020-07-03T10:29:34Z | - |
dc.date.available | 2020-07-03T10:29:34Z | - |
dc.date.issued | 2016 | en_US |
dc.identifier.issn | 1448-6083 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/26319 | - |
dc.description.abstract | We have compiled a catalogue of H ii regions detected with the Murchison Widefield Array between 72 and 231 MHz. The multiple frequency bands provided by the Murchison Widefield Array allow us identify the characteristic spectrum generated by the thermal Bremsstrahlung process in H ii regions. We detect 306 H ii regions between 260° < l < 340° and report on the positions, sizes, peak, integrated flux density, and spectral indices of these H ii regions. By identifying the point at which H ii regions transition from the optically thin to thick regime, we derive the physical properties including the electron density, ionised gas mass, and ionising photon flux, towards 61 H ii regions. This catalogue of H ii regions represents the most extensive and uniform low frequency survey of H ii regions in the Galaxy to date. | en_US |
dc.language.iso | eng | en_US |
dc.title | A Large-Scale, Low-Frequency Murchison Widefield Array Survey of Galactic H ii Regions between 260 < l < 340 | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1017/pasa.2016.19 | en_US |
dc.identifier.scopus | 2-s2.0-84969262584 | en_US |
dc.identifier.isi | 000376681900001 | en_US |
dc.identifier.url | https://www.cambridge.org/core/journals/publications-of-the-astronomical-society-of-australia/article/largescale-lowfrequency-murchison-widefield-array-survey-of-galactic-h-ii-regions-between-260-l-340/730F44B31EBE12ED8F24D114916BA127 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 33 | en_US |
dc.relation.firstpage | e020 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | USA | en_US |
dc.contributor.country | AUS | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2016PASA...33...20H | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Article | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | reserved | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.orcid | 0000-0002-0916-7443 | - |
crisitem.journal.journalissn | 1448-6083 | - |
crisitem.journal.ance | E211088 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | Existing users please |
---|---|---|---|---|
PASA postprint1605.02872.pdf | postprint | 2.92 MB | Adobe PDF | |
Hindson2016.pdf | [Administrators only] | 1.1 MB | Adobe PDF |
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