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Title: | Torque reversals and pulse profile of the pulsar 4U 1626-67 |
Authors: | Beri, Aru Jain, Chetana Paul, Biswajit Raichur, Harsha |
Keywords: | accretion discs |
Issue Date: | 1-Apr-2014 |
Publisher: | Oxford University Press |
Citation: | Monthly Notices of the Royal Astronomical Society, 2014, Vol. 439, p1940-1947 |
Abstract: | We review the pulse profile evolution of the unique accretion powered X-ray pulsar 4U 1626−67 over the last 40 yr since its discovery. This pulsar showed two distinct eras of steady spin-up separated by a steady spin-down episode for about 18 yr. In this work, using data from different observatories active during each phase of spin-up and spin-down, we establish a clear correlation between the accretion torque acting on this pulsar and its pulse profile. The energy-resolved pulse profiles are identical in both the spin-up eras and quite different in the spin-down era, especially in the low-energy band. This correlation, along with the already known feature of strong quasi-periodic oscillations (QPO) that was present only in the spin-down era, clearly establishes two different accretion modes on to the neutron star which produce different pulse profiles and only one of which produces the QPOs. |
Description: | Open Access |
URI: | http://hdl.handle.net/2289/5959 |
ISSN: | 0035-8711 1365-2966 - (online) |
Alternative Location: | http://adsabs.harvard.edu/abs/2014MNRAS.439.1940B http://arxiv.org/abs/1401.2936 http://dx.doi.org/10.1093/mnras/stu087 |
Copyright: | 2014 The authors & the Royal Astronomical Society. |
Appears in Collections: | Research Papers (A&A) |
Files in This Item:
File | Description | Size | Format | |
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2014_MNRAS_439_1940.pdf | Open Access | 923.08 kB | Adobe PDF | View/Open |
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