Sco X‐1: Hints of Periodic Variability at Radio Frequencies
Open Access
- 20 May 1997
- journal article
- research article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 481 (1) , 489-499
- https://doi.org/10.1086/304029
Abstract
We present the results of the flux density variability observations of Sco X-1 obtained during six VLA observing sessions between 1981 and 1990. The light curves indicate three timescales of flux density variation: slow, intermediate, and rapid. The rapidity of the variations sets a conservative upper limit on size of ~6 mas, assuming a distance of 200 pc, from light travel arguments for the radio-emitting regions. The corresponding brightness temperature of greater than 107 K indicates a nonthermal origin for the radio emission. A detailed analysis of the light curves suggests that the radio emission may exhibit true periodicity on timescales of ~3 hr. We also provide a prescription for accurate signal recovery and image restoration of point and extended sources when an object of varying signal is present in the synthesized beam.Keywords
This publication has 19 references indexed in Scilit:
- The radio 'lobes' of Scorpius X-1 are unrelated background sourcesThe Astrophysical Journal, 1991
- Radio and X-ray states in the X-ray binary Scorpius X-1The Astrophysical Journal, 1990
- Numerical simulation of nonaxisymmetric adiabatic accretion flowThe Astrophysical Journal, 1988
- The 1982 September radio outburst of Cygnus X-3 - Evidence for jetlike emission expanding at not less than about 0.35 CThe Astrophysical Journal, 1983
- On the use of windows for harmonic analysis with the discrete Fourier transformProceedings of the IEEE, 1978
- Least-squares frequency analysis of unequally spaced dataAstrophysics and Space Science, 1976
- The spectroscopic binary Scorpius X-1The Astrophysical Journal, 1975
- A 'Twin-Exhaust' Model for Double Radio SourcesMonthly Notices of the Royal Astronomical Society, 1974
- The Nature of the First Cygnus X-3 Radio OutburstNature Physical Science, 1972
- The Frequency Splitting of Transient Solar Radio BurstsPublications of the Astronomical Society of Australia, 1969