Show simple item record

dc.contributor.authorZampieri, L.
dc.contributor.authorImpiombato, D.
dc.contributor.authorFalomo, R.
dc.contributor.authorGrise', F.
dc.contributor.authorSoria, Roberto
dc.date.accessioned2017-01-30T13:43:31Z
dc.date.available2017-01-30T13:43:31Z
dc.date.created2015-03-03T20:17:46Z
dc.date.issued2012
dc.identifier.citationZampieri, 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.urihttp://hdl.handle.net/20.500.11937/34443
dc.identifier.doi10.1111/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.publisherWiley-Blackwell Publishing Ltd.
dc.titleSearching for the orbital period of the ultraluminous X-ray source NGC 1313 X-2
dc.typeJournal Article
dcterms.source.volume419
dcterms.source.startPage1331
dcterms.source.endPage1337
dcterms.source.issn1365-2966
dcterms.source.titleMonthly 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.departmentCurtin Institute of Radio Astronomy (Physics)
curtin.accessStatusOpen access


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record