RRI Banner

Low frequency quasi-periodic oscillations in the hard X-ray emission from Cygnus X-1

dc.contributor.authorPaul, Biswajit
dc.contributor.authorAgrawal, P C
dc.contributor.authorRao, A R
dc.date.accessioned2012-07-13T06:24:03Z
dc.date.available2012-07-13T06:24:03Z
dc.date.issued1998-12
dc.descriptionRestricted Accessen
dc.description.abstractThe observations of the black hole binary Cygnus X-1 were made in the energy band of 20 - 100 keV with a balloon-borne Xenon-filled multiwire proportional counter telescope on 5th April 1992. Timing analysis of the data revealed the presence of quasi-periodic oscillations (QPO) in the hard X-ray emission from the source. The QPO feature in the power density spectrum is broad with a peak at a frequency of 0.06 Hz. This result is compared with similar reports of QPOs in Cyg X-1 in soft and hard X-rays. Short time scale random intensity variations in the X-ray light curve are described with a shot noiuse model.en
dc.identifier.citationJournal of Astrophysics and Astronomy, 1998, Vol. 19, p55-61en
dc.identifier.issn0250-6335
dc.identifier.issn0973-7758 (Online)
dc.identifier.urihttp://hdl.handle.net/2289/4881
dc.language.isoenen
dc.publisherIndian Academy of Sciences, Bangalore, Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1998JApA...19...55Pen
dc.relation.urihttp://dx.doi.org/10.1007/BF02714891en
dc.rights1998 Indian Academy of Sciences, Bangalore, Indiaen
dc.titleLow frequency quasi-periodic oscillations in the hard X-ray emission from Cygnus X-1en
dc.typeArticleen

Files