Issue |
A&A
Volume 540, April 2012
|
|
---|---|---|
Article Number | L4 | |
Number of page(s) | 3 | |
Section | Letters | |
DOI | https://doi.org/10.1051/0004-6361/201218883 | |
Published online | 28 March 2012 |
Period doubling and non-linear resonance in the black hole candidate IGR J17091-3624?
1
Experimental Study Group, Massachusetts Institute of
Technology, 77 Massachusetts
Avenue, 02139
Cambridge ( MA), USA
e-mail: pao@space.mit.edu
2
Copernicus Astronomical Center, ul. Bartycka 18, 00-716
Warszawa,
Poland
e-mail: wlodek@camk.edu.pl; pam@camk.edu.pl
3
Department of Physics, University of Gothenburg,
412-96
Göteborg,
Sweden
e-mail: marek.abramowicz@physics.gu.se
4
Institute of Physics, Faculty of Philosophy and Science, Silesian
University in Opava, Bezručovo nám.
13, 746-01
Opava, Czech
Republic
Received:
25
January
2012
Accepted:
10
March
2012
The two high frequency quasi periodic oscillations (HFQPOs) recently reported in the black hole candidate IGR J17091-3624 are in a 5:2 frequency ratio (164 Hz to 66 Hz). This ratio is strongly suggestive of period doubling and nonlinear resonance analogous to phenomena known in RV Tauri-type pulsating stars (and recently discovered also in oscillations of RR Lyrae-type and of BL Herculis-type variables). An interpretation of the frequency ratio in terms of nonlinear interactions and a comparison with the HFQPOs reported in GRS 1915+105 may imply a mass of about six solar masses for the black hole in IGR J17091-3624.
Key words: accretion, accretion disks / black hole physics / X-rays: binaries / asteroseismology
© ESO, 2012
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