Other
Scientific paper
Dec 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...20510405r&link_type=abstract
American Astronomical Society Meeting 205, #104.05; Bulletin of the American Astronomical Society, Vol. 36, p.1516
Other
2
Scientific paper
We first focus on 350 RXTE observations of GRS1915+105 while the source is in quasi-steady states (rms < 16% of mean in 1 s bins at 2-30 keV). The great majority of these are either in the hard state with detectable radio emission, or in a thermal state that is radio quiet. The 67 Hz QPO is seen in the thermal state, when the source enters a particular region of the color-color diagram. The correlation with X-ray flux is substantially weaker.
The other high-frequency QPOs (113 and 168 Hz) in GRS1915+105 are only seen by dissecting light curves for particular types of variable states. We review the spectral properties associated with these oscillations. They resemble the high-frequency QPOs in other black hole binaries, unlike the 67 Hz QPO.
Gazak Zachary J.
Lin Dacheng
Morgan Edward Harrington
Pooley Guy G.
Remillard Ron A.
No associations
LandOfFree
The 67 Hz QPO and Other High-Frequenecy Oscillations from the Black Hole Binary GRS1915+105 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The 67 Hz QPO and Other High-Frequenecy Oscillations from the Black Hole Binary GRS1915+105, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The 67 Hz QPO and Other High-Frequenecy Oscillations from the Black Hole Binary GRS1915+105 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1642144