X-ray Binaries - An Overview

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Binary Orbit CM M2 M1 a Compact star mass = M 1 M Normal star mass = M 2 M Binary separation = a, mass ratio q = M 2 /M 1 + Kepler' s law : 2 4π a 3 = G( M 1 + M 2 ) M Θ P 2 10 1/3 1 a = 3.5× 10 M (1 + q) 1/3 P 2/3 hr cm
Geometry Observed phenomenology depends on viewing angle.
Page 1 and 2: X-RAY BINARIES M.C. RAMADEVI ISRO S
Page 3 and 4: THIS IS A BINARY SYSTEM WITH NEUTRO
Page 5 and 6: X-ray emission What could possibly
Page 7 and 8: Two mechanisms of mass transfer in
Page 9 and 10: Classification of X-ray Binaries Hi
Page 11 and 12: X-ray Pulsars - Pulsations THIS IS
Page 13 and 14: Type I Bursts Observation of thermo
Page 15 and 16: Accretion onto black holes There is
Page 17 and 18: Variabilities observed in Black Hol
Page 19 and 20: Soft state
Page 21 and 22: Example An outburst observed in 4U
Page 23 and 24: Why study X-ray Binaries? To unders
Page 25 and 26: India’s first multi-wavelength AS
Page 28 and 29: LMXB •For NS, there is emission f
Page 32 and 33: Typical X-ray bursts: • 10 36 -10
Page 34: X-Ray Pulsar Cen X-3 Pulses are mod

X-ray Binaries - An Overview

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