2008ApJ...686..520Z

Query : 2008ApJ...686..520Z

2008ApJ...686..520Z - Astrophys. J., 686, 520-527 (2008/October-2)

The long-term radiative evolution of anomalous X-ray pulsar 1E 2259+586 after its 2002 outburst.

ZHU W., KASPI V.M., DIB R., WOODS P.M., GAVRIIL F.P. and ARCHIBALD A.M.

Abstract (from CDS):

We present an analysis of five XMM-Newton observations of the anomalous X-ray pulsar (AXP) 1E 2259+586 taken in 2004 and 2005 during its relaxation following its 2002 outburst. We compare these data with those of five previous XMM-Newton observations taken in 2002 and 2003, and find the observed flux decay is well described by a power law of index -0.69±0.03. As of mid-2005, the source may still have been brighter than preoutburst, and was certainly hotter. We find a strong correlation between hardness and flux, as seen in other AXPs. We discuss the implications of these results for the magnetar model.

Abstract Copyright: ∼

Journal keyword(s): Stars: Pulsars: Individual: Alphanumeric: 1E 2259+586 - Stars: Neutron - X-Rays: Stars

Simbad objects: 10

goto Full paper

goto View the references in ADS

Number of rows : 10
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 2E 2336 HXB 10 50 08.93 -59 53 19.9           Be 419 0
2 GRB 980618A gB 16 35 52 -47 35.2           ~ 270 0
3 PSR J1647-4552 Psr 16 47 10.18 -45 52 16.7           ~ 217 1
4 PSR J1708-4008 Psr 17 08 46.1 -40 08 56           ~ 315 0
5 AX J1809.8-1943 Psr 18 09 51.07 -19 43 51.8           ~ 532 0
6 PSR J1841-0456 Psr 18 41 19.29 -04 56 11.4           ~ 296 1
7 AX J1844.8-0258 HXB 18 44 53 -02 56.0           ~ 126 0
8 GBS 1900+14 gB 19 07 13 +09 19.6           ~ 906 0
9 2E 4673 HXB 23 01 08.14 +58 52 44.5           ~ 673 1
10 SNR G109.1-01.0 SNR 23 01 35 +58 53.0           ~ 362 0

To bookmark this query, right click on this link: simbad:objects in 2008ApJ...686..520Z and select 'bookmark this link' or equivalent in the popup menu