A large-scale, low-frequency murchison widefield array survey of galactic H II regions between 260 < l < 340
Hindson, L
Johnston-Hollitt, M
Hurley-Walker, N
Callingham, JR
Su, H
Morgan, J
Bell, M
Bernardi, G
Bowman, JD
Briggs, F
Cappallo, RJ
Deshpande, AA
Dwarakanath, KS
For, BQ
Gaensler, BM
Greenhill, LJ
Hancock, P
Hazelton, BJ
Kapinska, AD
Kaplan, DL
Lenc, E
Lonsdale, CJ
Mckinley, B
McWhirter, SR
Mitchell, DA
Morales, MF
Morgan, E
Oberoi, D
Offringa, A
Ord, SM
Procopio, P
Prabu, T
Udaya Shankar, N
Srivani, KS
Staveley-Smith, L
Subrahmanyan, R
Tingay, SJ
Wayth, RB
Webster, RL
Williams, A
Williams, CL
Wu, C
Zheng, Q
- Publication Type:
- Journal Article
- Citation:
- Publications of the Astronomical Society of Australia, 2016, 33
- Issue Date:
- 2016-05-17
Closed Access
Filename | Description | Size | |||
---|---|---|---|---|---|
largescale_lowfrequency_murchison_widefield_array_survey_of_galactic_h_ii_regions_between_260_l_340.pdf | Published Version | 1.1 MB | Adobe PDF |
Copyright Clearance Process
- Recently Added
- In Progress
- Closed Access
This item is closed access and not available.
Full metadata record
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, JR | en_US |
dc.contributor.author | Su, H | en_US |
dc.contributor.author | Morgan, J | en_US |
dc.contributor.author |
Bell, M https://orcid.org/0000-0003-1767-5277 |
en_US |
dc.contributor.author | Bernardi, G | en_US |
dc.contributor.author | Bowman, JD | en_US |
dc.contributor.author | Briggs, F | en_US |
dc.contributor.author | Cappallo, RJ | en_US |
dc.contributor.author | Deshpande, AA | en_US |
dc.contributor.author | Dwarakanath, KS | en_US |
dc.contributor.author | For, BQ | en_US |
dc.contributor.author | Gaensler, BM | en_US |
dc.contributor.author | Greenhill, LJ | en_US |
dc.contributor.author | Hancock, P | en_US |
dc.contributor.author | Hazelton, BJ | en_US |
dc.contributor.author | Kapinska, AD | en_US |
dc.contributor.author | Kaplan, DL | en_US |
dc.contributor.author | Lenc, E | en_US |
dc.contributor.author | Lonsdale, CJ | en_US |
dc.contributor.author | Mckinley, B | en_US |
dc.contributor.author | McWhirter, SR | en_US |
dc.contributor.author | Mitchell, DA | en_US |
dc.contributor.author | Morales, MF | 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, SM | en_US |
dc.contributor.author | Procopio, P | en_US |
dc.contributor.author | Prabu, T | en_US |
dc.contributor.author | Udaya Shankar, N | en_US |
dc.contributor.author | Srivani, KS | en_US |
dc.contributor.author | Staveley-Smith, L | en_US |
dc.contributor.author | Subrahmanyan, R | en_US |
dc.contributor.author | Tingay, SJ | en_US |
dc.contributor.author | Wayth, RB | en_US |
dc.contributor.author | Webster, RL | en_US |
dc.contributor.author | Williams, A | en_US |
dc.contributor.author | Williams, CL | en_US |
dc.contributor.author | Wu, C | en_US |
dc.contributor.author | Zheng, Q | en_US |
dc.date.issued | 2016-05-17 | en_US |
dc.identifier.citation | Publications of the Astronomical Society of Australia, 2016, 33 | en_US |
dc.identifier.issn | 1323-3580 | en_US |
dc.identifier.uri | http://hdl.handle.net/10453/113565 | |
dc.description.abstract | © Astronomical Society of Australia 2016. 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.relation.ispartof | Publications of the Astronomical Society of Australia | en_US |
dc.relation.isbasedon | 10.1017/pasa.2016.19 | en_US |
dc.subject.classification | Astronomy & Astrophysics | 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 | Journal Article | |
utslib.citation.volume | 33 | en_US |
utslib.for | 0201 Astronomical and Space Sciences | en_US |
utslib.for | 0299 Other Physical Sciences | en_US |
pubs.embargo.period | Not known | en_US |
pubs.organisational-group | /University of Technology Sydney | |
pubs.organisational-group | /University of Technology Sydney/Faculty of Science | |
pubs.organisational-group | /University of Technology Sydney/Faculty of Science/School of Mathematical and Physical Sciences | |
utslib.copyright.status | closed_access | |
pubs.publication-status | Published | en_US |
pubs.volume | 33 | en_US |
Abstract:
© Astronomical Society of Australia 2016. 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.
Please use this identifier to cite or link to this item:
Download statistics for the last 12 months
Not enough data to produce graph