z-logo
open-access-imgOpen Access
Long‐Term X‐Ray Variability in GX 13+1: Energy‐dependent Periodic Modulation
Author(s) -
R. H. D. Corbet
Publication year - 2003
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/377469
Subject(s) - modulation (music) , physics , astrophysics , period (music) , flux (metallurgy) , spectral line , noise (video) , line (geometry) , energy (signal processing) , signal (programming language) , optics , materials science , astronomy , mathematics , geometry , artificial intelligence , computer science , acoustics , metallurgy , image (mathematics) , quantum mechanics , programming language
A search is made for periodic modulation in the X-ray flux from the low massX-ray binary GX13+1 using Rossi X-ray Timing Explorer All Sky Monitor datacollected over a period of almost seven years. From a filtered data set, whichexcludes measurements with exceptionally large error bars and so maximizessignal to noise, modulation is found at a period of 24.065 +/- 0.018 days. Themodulation is most clearly detectable at high energies (5 - 12 keV). Spectralchanges are revealed as a modulation in hardness ratio on the 24 day period andthere is a phase shift between the modulation in the 5 - 12 keV energy bandcompared to the 1.5 - 5 keV band. The high-energy spectrum of GX13+1 is unusualin displaying both emission and absorption iron line features and it isspeculated that the peculiar spectral and timing properties may be connected.Comment: Accepted for publication in ApJ. 21 pages including 9 figure

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom