Esposito, P;
Burgay, M;
Possenti, A;
Turolla, R;
Zane, S;
De Luca, A;
Tiengo, A;
... Rea, N; + view all
(2009)
Spin-down rate and inferred dipole magnetic field of the soft gamma-ray repeater SGR 1627-41.
Monthly Notices of the Royal Astronomical Society
, 399
(1)
L44 - L48.
10.1111/j.1745-3933.2009.00723.x.
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Abstract
Using Chandra data taken in 2008 June, we detected pulsations at 2.594 39(4) s in the soft gamma-ray repeater SGR 1627−41. This is the second measurement of the source spin period and allows us to derive for the first time a long-term spin-down rate of (1.9 ± 0.4) × 10−11 s s−1. From this value, we infer for SGR 1627−41 a characteristic age of ∼2.2 kyr, a spin-down luminosity of ∼4 × 1034 erg s−1 (one of the highest among sources of the same class), and a surface dipole magnetic field strength of ∼2 × 1014 G. These properties confirm the magnetar nature of SGR 1627−41; however, they should be considered with caution since they were derived on the basis of a period derivative measurement made using two epochs only, and magnetar spin-down rates are generally highly variable. The pulse profile, double-peaked and with a pulsed fraction of 13 ± 2 per cent in the 2–10 keV range, closely resembles that observed by XMM–Newton in 2008 September. Having for the first time a timing model for this soft gamma-ray repeater (SGR), we also searched for a pulsed signal in archival radio data collected with the Parkes radio telescope 9 months after the previous X-ray outburst. No evidence for radio pulsations was found, down to a luminosity level ∼10–20 times fainter (for a 10 per cent duty cycle and a distance of 11 kpc) than the peak luminosity shown by the known radio magnetars.
Type: | Article |
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Title: | Spin-down rate and inferred dipole magnetic field of the soft gamma-ray repeater SGR 1627-41 |
Open access status: | An open access version is available from UCL Discovery |
DOI: | 10.1111/j.1745-3933.2009.00723.x |
Publisher version: | http://dx.doi.org/10.1111/j.1745-3933.2009.00723.x |
Language: | English |
Additional information: | © 2009 RAS Definitive versions of articles pre-2013 are available at http://onlinelibrary.wiley.com/journal/10.1111/(ISSN)1365-2966, now published by http://mnras.oxfordjournals.org |
Keywords: | stars: neutron, pulsars: general, X-rays: individual: SGR1627-41 |
UCL classification: | UCL UCL > Provost and Vice Provost Offices > UCL BEAMS UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics |
URI: | https://discovery-pp.ucl.ac.uk/id/eprint/178098 |
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