AMI limits on 15-GHz excess emission in northern HII regions
We present observations between 14.2 and 17.9 GHz of 16 Galactic H II regions made withthe Arcminute Microkelvin Imager. In conjunction with data from the literature at lower radiofrequencies we investigate the possibility of a spinning dust component in the spectra of theseobjects. We conclude that...
| Main Authors: | , , , , , , , , , , , , , , , |
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| Format: | Journal Article |
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Oxford University Press
2008
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| Subjects: | |
| Online Access: | http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?2008MNRAS.385..809S&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf http://hdl.handle.net/20.500.11937/26297 |
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| author | Scaife, A. Hurley-Walker, Natasha Davies, M. Duffett-Smith, P. Feroz, F. Grainge, K. Green, D. Hobson, M. Kaneko, T. Lasenby, A. Pooley, G. Saunders, R. Scott, P. Titterington, D. Waldram, E. Zwart, J. |
| author_facet | Scaife, A. Hurley-Walker, Natasha Davies, M. Duffett-Smith, P. Feroz, F. Grainge, K. Green, D. Hobson, M. Kaneko, T. Lasenby, A. Pooley, G. Saunders, R. Scott, P. Titterington, D. Waldram, E. Zwart, J. |
| author_sort | Scaife, A. |
| building | Curtin Institutional Repository |
| collection | Online Access |
| description | We present observations between 14.2 and 17.9 GHz of 16 Galactic H II regions made withthe Arcminute Microkelvin Imager. In conjunction with data from the literature at lower radiofrequencies we investigate the possibility of a spinning dust component in the spectra of theseobjects. We conclude that there is no signi?cant evidence for spinning dust towards thesesources and measure an average spectral index of a = 0.15 ± 0.07 (where S ? ?-a) between1.4 and 17.9 GHz for the sample. |
| first_indexed | 2025-11-14T08:00:48Z |
| format | Journal Article |
| id | curtin-20.500.11937-26297 |
| institution | Curtin University Malaysia |
| institution_category | Local University |
| last_indexed | 2025-11-14T08:00:48Z |
| publishDate | 2008 |
| publisher | Oxford University Press |
| recordtype | eprints |
| repository_type | Digital Repository |
| spelling | curtin-20.500.11937-262972017-02-28T01:49:15Z AMI limits on 15-GHz excess emission in northern HII regions Scaife, A. Hurley-Walker, Natasha Davies, M. Duffett-Smith, P. Feroz, F. Grainge, K. Green, D. Hobson, M. Kaneko, T. Lasenby, A. Pooley, G. Saunders, R. Scott, P. Titterington, D. Waldram, E. Zwart, J. ISM: clouds radio continuum: ISM radiation mechanisms: thermal H II regions We present observations between 14.2 and 17.9 GHz of 16 Galactic H II regions made withthe Arcminute Microkelvin Imager. In conjunction with data from the literature at lower radiofrequencies we investigate the possibility of a spinning dust component in the spectra of theseobjects. We conclude that there is no signi?cant evidence for spinning dust towards thesesources and measure an average spectral index of a = 0.15 ± 0.07 (where S ? ?-a) between1.4 and 17.9 GHz for the sample. 2008 Journal Article http://hdl.handle.net/20.500.11937/26297 http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?2008MNRAS.385..809S&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf Oxford University Press restricted |
| spellingShingle | ISM: clouds radio continuum: ISM radiation mechanisms: thermal H II regions Scaife, A. Hurley-Walker, Natasha Davies, M. Duffett-Smith, P. Feroz, F. Grainge, K. Green, D. Hobson, M. Kaneko, T. Lasenby, A. Pooley, G. Saunders, R. Scott, P. Titterington, D. Waldram, E. Zwart, J. AMI limits on 15-GHz excess emission in northern HII regions |
| title | AMI limits on 15-GHz excess emission in northern HII regions |
| title_full | AMI limits on 15-GHz excess emission in northern HII regions |
| title_fullStr | AMI limits on 15-GHz excess emission in northern HII regions |
| title_full_unstemmed | AMI limits on 15-GHz excess emission in northern HII regions |
| title_short | AMI limits on 15-GHz excess emission in northern HII regions |
| title_sort | ami limits on 15-ghz excess emission in northern hii regions |
| topic | ISM: clouds radio continuum: ISM radiation mechanisms: thermal H II regions |
| url | http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?2008MNRAS.385..809S&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf http://hdl.handle.net/20.500.11937/26297 |