Issue |
A&A
Volume 591, July 2016
|
|
---|---|---|
Article Number | A36 | |
Number of page(s) | 6 | |
Section | Astrophysical processes | |
DOI | https://doi.org/10.1051/0004-6361/201527711 | |
Published online | 07 June 2016 |
Impact of inclination on quasi-periodic oscillations from spiral structures
1
AstroParticule & Cosmologie (APC), UMR 7164, Université Paris
Diderot,
10 rue Alice Domon et Leonie Duquet,
75205
Paris Cedex 13,
France
e-mail:
varniere@apc.univ-paris7.fr
2
Observatoire de Paris/LESIA, 5 place Jules Janssen, 92195
Meudon Cedex,
France
3
Nicolaus Copernicus Astronomical Center, ul. Bartycka
18, 00-716
Warszawa,
Poland
Received: 6 November 2015
Accepted: 18 March 2016
Context. Quasi-periodic oscillations (QPOs) are a common feature of the power spectrum of X-ray binaries. Currently it is not possible to unambiguously differentiate the large number of proposed models to explain these phenomena through existing observations.
Aims. We investigate the observable predictions of a simple model that generates flux modulation: a spiral instability rotating in a thin accretion disk. This model is motivated by the accretion ejection instability (AEI) model for low-frequency QPOs (LFQPOs). We are particularly interested in the inclination dependence of the observables that are associated with this model.
Methods. We develop a simple analytical model of an accretion disk, which features a spiral instability. The disk is assumed to emit blackbody radiation, which is ray-traced to a distant observer. We compute pulse profiles and power spectra as observed from infinity.
Results. We show that the amplitude of the modulation associated with the spiral rotation is a strong function of inclination and frequency. The pulse profile is quasi-sinusoidal only at low inclination (face-on source). As a consequence, a higher-inclination geometry leads to a stronger and more diverse harmonic signature in the power spectrum.
Conclusions. We present how the amplitude depends on the inclination when the flux modulation comes from a spiral in the disk. We also include new observables that could potentially differentiate between models, such as the pulse profile and the harmonic content of the power spectra of high-inclination sources that exhibit LFQPOs. These might be important observables to explore with existing and new instruments.
Key words: X-rays: binaries / accretion, accretion disks / instabilities
© ESO, 2016
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.