High energy X-ray timing and spectral observations of SCO X-1, CYG X-1, GX 5-1, CYG X-3 and GX 1+4

Author:

Damle S.V.,Kunte P.K.,Leahy D.A.,Naranan S.,Sreekantan B.V.,Venkatesan D.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Aerospace Engineering,General Earth and Planetary Sciences,Atmospheric Science,Geophysics,Astronomy and Astrophysics

Reference9 articles.

1. A High Sensitivity Phoswich Scintillator X-Ray Telescope for Hard X-Ray (20–120 keV) Astronomy from Balloon Platform;Damle,1986

2. Comptonization of X-rays in Plasma Clouds;Syunyaev;Astron. Astrophys.,1980

3. Hard X-ray Observations of the Quasar 3C273;Damle;Astron. Astrophys. Letters,1987

4. On Searches for Pulsed Emission with Application to Four Globular Cluster X-ray Sources: NGC 1951, 6641, 6624, and 6712;Leahy;Ap. J.,1983

5. On Searches for Pulsed Emission: Improved Determination of Period and Amplitude from Epoch Folding for Sinusoidal Signals;Leahy;Astron. Ap.,1987

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2. Spin period evolution of GX 1+4;Astronomy & Astrophysics;2012-01

3. Correlated Radial Velocity and X‐Ray Variations in HD 154791/4U 1700+24;The Astrophysical Journal;2002-12

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5. A phoswich Anger camera for hard X-ray and low energy gamma-ray astronomy;Advances in Space Research;1996-01

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