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A torque reversal to spin-up in 4U 1626-67

dc.contributor.authorJain, Chetana
dc.contributor.authorPaul, Biswajit
dc.date.accessioned2009-07-29T11:30:23Z
dc.date.available2009-07-29T11:30:23Z
dc.date.issued2009-06-24
dc.descriptionOpen Accessen
dc.description.abstractWe report the detection of a recent torque reversal to spin-up in 4U 1626-67. This is an accretion powered X-ray pulsar and shows slow gradual intensity and pulse period variation on a few years of timescale. Recently, a significant increase in the X-ray flux was observed in the long term RXTE-ASM and Swift-BAT light curve (Krimm et al. 2008, ATel #1426, 1, Jain et al. 2009, astro-ph 0906.4169) around MJD 54500.en
dc.identifier.citationAstronomer's Telegram No.2095, 2009en
dc.identifier.urihttp://hdl.handle.net/2289/3813
dc.language.isoenen
dc.publisherATELen
dc.relation.urihttp://adsabs.harvard.edu/abs/2009ATel.2095....1Jen
dc.relation.urihttp://www.astronomerstelegram.org/?read=2095en
dc.rights2009 ATELen
dc.titleA torque reversal to spin-up in 4U 1626-67en
dc.typeArticleen

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