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    http://hdl.handle.net/2289/5959| 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 | |
|---|---|---|---|---|
| 2014_MNRAS_439_1940.pdf | Open Access | 923.08 kB | Adobe PDF | View/Open | 
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