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http://hdl.handle.net/2289/2710
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DC Field | Value | Language |
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dc.contributor.author | Kaur, Ramanpreet | - |
dc.contributor.author | Paul, Biswajit | - |
dc.contributor.author | Raichur, Harsha | - |
dc.contributor.author | Sagar, R. | - |
dc.date.accessioned | 2007-06-11T09:31:51Z | - |
dc.date.available | 2007-06-11T09:31:51Z | - |
dc.date.issued | 2007-05-10 | - |
dc.identifier.citation | Astrophysical Journal, 2007, Vol.660, p1409-1412 | en |
dc.identifier.issn | 0004-637X | - |
dc.identifier.issn | 1538-4357(Online) | - |
dc.identifier.uri | http://hdl.handle.net/2289/2710 | - |
dc.description | Restricted Access. An open-access version is available at arXiv.org. Articles older than 2 years are open to all at the journal site (alternative location) | en |
dc.description.abstract | We report the discovery of quasi-periodic oscillations (QPOs) in the high-mass X-ray binary (HMXB) pulsar XTE J0111.2-7317 during a transient outburst of the source in 1998 December. Using observations made with the Proportional Counter Array of the Rossi X-Ray Timing Explorer during the second peak and the declining phase of the outburst, we have discovered a QPO feature at a frequency of 1.27 Hz. We have ruled out the possibility that the observed feature could instead be from the neighboring bright X-ray pulsar SMC X-1. This is the highest frequency QPO ever detected in an HMXB pulsar. In the absence of a cyclotron absorption feature in the X-ray spectrum, the QPO, along with the pulse period and X-ray flux measurement, helps us to constrain the magnetic field strength of the neutron star. | en |
dc.format.extent | 183851 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | en |
dc.publisher | The American Astronomical Society | en |
dc.relation.uri | http://adsabs.harvard.edu/cgi-bin/bib_query?2007ApJ...660.1409K | en |
dc.relation.uri | http://arxiv.org/abs/astro-ph/0703205 | en |
dc.relation.uri | http://dx.doi.org/10.1086/513418 | en |
dc.rights | 2007 American Astronomical Society | en |
dc.subject | Stars: Binaries: General | en |
dc.subject | Stars: Pulsars: Individual: Alphanumeric: XTE J0111.2-7317 | en |
dc.subject | Stars: Neutron, X-Rays: Binaries | en |
dc.subject | X-rays: individual (XTE J0111.2-7317) | en |
dc.subject | X-Rays: Stars | en |
dc.title | Quasi-periodic oscillations in XTE J0111.2-7317: Highest frequency among the HMXB pulsars | en |
dc.type | Article | en |
Appears in Collections: | Research Papers (A&A) |
Files in This Item:
File | Description | Size | Format | |
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2007 APJ V660 p1409.pdf Restricted Access | Restricted Access | 179.54 kB | Adobe PDF | View/Open Request a copy |
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