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dc.contributor.authorHakala, P.
dc.contributor.authorWagner, R. M.
dc.contributor.authorStarrfield, S.
dc.contributor.authorNess, J. -U.
dc.contributor.authorBALMAN, Şölen
dc.contributor.authorBeardmore, A. P.
dc.contributor.authorOsborne, J. P.
dc.contributor.authorPage, K. L.
dc.contributor.authorSchwarz, G.
dc.date.accessioned2021-03-02T21:50:59Z
dc.date.available2021-03-02T21:50:59Z
dc.date.issued2010
dc.identifier.citationBeardmore A. P. , Osborne J. P. , Page K. L. , Schwarz G., Starrfield S., Hakala P., Ness J. -. , BALMAN Ş., Wagner R. M. , "Swift observations of CSS081007:030559+054715", ASTRONOMISCHE NACHRICHTEN, cilt.331, sa.2, ss.156-159, 2010
dc.identifier.issn0004-6337
dc.identifier.otherav_093fcf7e-7624-4c76-9258-c5d12715e0e4
dc.identifier.othervv_1032021
dc.identifier.urihttp://hdl.handle.net/20.500.12627/12028
dc.identifier.urihttps://doi.org/10.1002/asna.200911318
dc.description.abstractCSS081007:030559+054715 was discovered by the Catalina Real-time Transient Survey. Optical spectroscopy revealed a multi-peaked Ha emission line profile with radial velocities exceeding 1500 km/s, as well as strong Ne emission, suggestive of a neon nova. We monitored the source extensively with the Swift satellite, obtaining a unique dataset spanning 270 days in the soft X-ray and UV bands. The data reveal a soft, blackbody-like spectrum with a temperature around 55 eV (though dependent on the modelling), variable X-ray and UV light curves with a 1.77 day period in both the X-ray and UV bands, a longer timescale modulation of similar to 50 days, followed by a slowly declining trend in the soft X-ray and UV flux. We highlight the Swift observations and their implications for the SSS nature of this object. (C) 2010 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim
dc.language.isoeng
dc.subjectUzay bilimi
dc.subjectTemel Bilimler
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.subjectAstronomi ve Astrofizik
dc.subjectFizik
dc.subjectTemel Bilimler (SCI)
dc.titleSwift observations of CSS081007:030559+054715
dc.typeMakale
dc.relation.journalASTRONOMISCHE NACHRICHTEN
dc.contributor.departmentUniversity Of Leicester , ,
dc.identifier.volume331
dc.identifier.issue2
dc.identifier.startpage156
dc.identifier.endpage159
dc.contributor.firstauthorID2212574


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