Journal Article

On the harmonics of the low-frequency quasi-periodic oscillation in GRS 1915+105

E. M. Ratti, T. M. Belloni and S. E. Motta

in Monthly Notices of the Royal Astronomical Society

Published on behalf of The Royal Astronomical Society

Volume 423, issue 1, pages 694-701
Published in print June 2012 | ISSN: 0035-8711
Published online May 2012 | e-ISSN: 1365-2966 | DOI: http://dx.doi.org/10.1111/j.1365-2966.2012.20906.x
On the harmonics of the low-frequency quasi-periodic oscillation in GRS 1915+105

More Like This

Show all results sharing this subject:

  • Astronomy and Astrophysics

GO

Show Summary Details

Preview

GRS 1915+105 is a widely studied black hole binary, well known because of its extremely fast and complex variability. Flaring periods of high variability alternate with ‘stable’ phases (the plateaux) when the flux is low, the spectra are hard and the timing properties of the source are similar to those of a number of black hole candidates in the hard spectral state. In the plateaux the power density spectra (PDS) are dominated by a low-frequency quasi-periodic oscillation (LFQPO) superposed on to a band-limited noise continuum and accompanied by at least one harmonic. In this paper we focus on three plateaux, presenting the analysis of the PDS and in particular of the LFQPO and its harmonics. While plotting the LFQPO and all the harmonics together on a frequency–width plane, we found the presence of a positive trend of broadening when the frequency increases. This trend can shed light on the nature of the harmonic content of the LFQPO and challenges the usual interpretation of these timing features.

Keywords: accretion, accretion discs; X-rays: binaries; X-rays: individual: GRS 1915+105

Journal Article.  4126 words.  Illustrated.

Subjects: Astronomy and Astrophysics

Full text: subscription required

How to subscribe Recommend to my Librarian

Users without a subscription are not able to see the full content. Please, subscribe or login to access all content.