Searching for the orbital period of the ultraluminous X-ray source NGC 1313 X-2
| dc.contributor.author | Zampieri, L. | |
| dc.contributor.author | Impiombato, D. | |
| dc.contributor.author | Falomo, R. | |
| dc.contributor.author | Grise', F. | |
| dc.contributor.author | Soria, Roberto | |
| dc.date.accessioned | 2017-01-30T13:43:31Z | |
| dc.date.available | 2017-01-30T13:43:31Z | |
| dc.date.created | 2015-03-03T20:17:46Z | |
| dc.date.issued | 2012 | |
| dc.identifier.citation | Zampieri, L. and Impiombato, D. and Falomo, R. and Grise', F. and Soria, R. 2012. Searching for the orbital period of the ultraluminous X-ray source NGC 1313 X-2. Monthly Notices of the Royal Astronomical Society. 419: pp. 1331-1337. | |
| dc.identifier.uri | http://hdl.handle.net/20.500.11937/34443 | |
| dc.identifier.doi | 10.1111/j.1365-2966.2011.19790.x | |
| dc.description.abstract |
We analysed the longest phase-connected photometric data set available for NGC 1313 X-2, looking for the ~6-day modulation reported by Liu et al.. The folded B-band light curve shows a ~6-day periodicity with a significance slightly larger than 3σ. The low statistical significance of this modulation, along with the lack of detection in the V band, makes its identification uncertain. | |
| dc.publisher | Wiley-Blackwell Publishing Ltd. | |
| dc.title | Searching for the orbital period of the ultraluminous X-ray source NGC 1313 X-2 | |
| dc.type | Journal Article | |
| dcterms.source.volume | 419 | |
| dcterms.source.startPage | 1331 | |
| dcterms.source.endPage | 1337 | |
| dcterms.source.issn | 1365-2966 | |
| dcterms.source.title | Monthly Notices of the Royal Astronomical Society | |
| curtin.note |
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society, ©: 2011, the authors and the Royal Astronomical Society. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. | |
| curtin.department | Curtin Institute of Radio Astronomy (Physics) | |
| curtin.accessStatus | Open access |