2002ApJ...577..929G


Query : 2002ApJ...577..929G

2002ApJ...577..929G - Astrophys. J., 577, 929-939 (2002/October-1)

A comprehensive study of pulse profile evolution in SGR 1806-20 and SGR 1900+14 with the Rossi X-ray timing explorer proportional counter array.

GOGUS E., KOUVELIOTOU C., WOODS P.M., FINGER M.H. and VAN DER KLIS M.

Abstract (from CDS):

Soft gamma repeaters undergo pulse profile changes in connection with their burst activity. Here we present a comprehensive pulse profile history of SGR 1806-20 and SGR 1900+14 in three energy bands using Rossi X-Ray Timing Explorer/Proportional Counter Array observations performed between 1996 and 2001. Using the Fourier harmonic powers of pulse profiles, we quantify the pulse shape evolution. Moreover, we determined the rms pulsed count rates (PCRs) of each profile. We show that the pulse profiles of SGR 1806-20 remain single pulsed, showing only modest changes for most of our observing span, while those of SGR 1900+14 change remarkably in all energy bands. Highly significant pulsations from SGR 1900+14 following the 1998 August 27 and 2001 April 18 bursts enabled us to study not only the decay of PCRs in different energy bands but also their correlations with each other.

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Journal keyword(s): Stars: Individual: Alphanumeric: SGR 1806-20 - Stars: Individual: Alphanumeric: SGR 1900+14

Simbad objects: 5

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Number of rows : 5
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 PSR B0525-66 Psr 05 26 00.7 -66 04 35           ~ 569 1
2 PSR J1808-2024 Psr 18 08 39.32 -20 24 40.1           ~ 1316 2
3 2MASS J19044747+0902419 HXB 19 04 47.4654450192 +09 02 41.756177328           Be? 32 0
4 GBS 1900+14 gB 19 07 13 +09 19.6           ~ 906 0
5 4U 1907+09 HXB 19 09 38.0514267264 +09 49 47.270139132   19.41 16.35 15.570 12.53 O9.5Iab 362 0

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