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Existing Transient Surveys: High Energy II: X-ray Binaries. Geoff Bower. Discovery of X-ray Stars. Giacconi et al 1962. Aerobee Rocket. Designed by James van Allen Aerojet booster Bumblebee second stage Maximum altitude of 225 km Above 80 km for 350 seconds Traveled for 120 km.
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Existing Transient Surveys:High Energy II:X-ray Binaries Geoff Bower The Transient Universe: AY 250 Spring 2007
Discovery of X-ray Stars Giacconi et al 1962 The Transient Universe: AY 250 Spring 2007
Aerobee Rocket • Designed by James van Allen • Aerojet booster • Bumblebee second stage • Maximum altitude of 225 km • Above 80 km for 350 seconds • Traveled for 120 km The Transient Universe: AY 250 Spring 2007
New Detectors • Geiger counters • Greater collecting area • Anti-coincidence shields • 50-100 times more sensitive than solar X-ray experiments The Transient Universe: AY 250 Spring 2007
Sco X-1 No optical counterpart known Eventually 13th mag Lx ~ 10^3 Lopt Radio counterparts expected X-ray background detected Earth origin? Two Discoveries The Transient Universe: AY 250 Spring 2007
Two Sources Discovered Giacconi et al 1964 The Transient Universe: AY 250 Spring 2007
More Sources Found • SNR • Nearby AGN • Galactic sources Rossi 1967 The Transient Universe: AY 250 Spring 2007
Characterizing Sco X-1 • Some variability • X-ray • Optical • 1000 x energy in X-rays than any other band • Thermal spectrum 50 x 10^6 K • Atomic lines in optical • No clear understanding in early days The Transient Universe: AY 250 Spring 2007
Pulsations & Occultations ~ 4 Seconds R < 10^9 cm Schreier et al 1972 The Transient Universe: AY 250 Spring 2007
Binary Model Mx ~ 1 Msun M* ~ 17 – 46 Msun The Transient Universe: AY 250 Spring 2007
Periodic Fluctuations Bursts of X-ray emission following accretion Masses exceeding 3 Msun Neutron Star & Black Hole Binaries The Transient Universe: AY 250 Spring 2007
Low mass companion (< 10 Msun) Star overfills its Roche lobe Lifetime – 10^7 – 10^9 y High mass companion Stellar wind drives mass accretion Lifetimes < 10^7 y LMXB & HMXB Only hundreds in the entire galaxy Dozens known The Transient Universe: AY 250 Spring 2007
Galactic Distribution O LMXB * HMXB Grimm et al 2002 The Transient Universe: AY 250 Spring 2007
Galactic Distribution The Transient Universe: AY 250 Spring 2007
Luminosity Distributions The Transient Universe: AY 250 Spring 2007
Super-Eddington Accretors The Transient Universe: AY 250 Spring 2007
GRS 1915+105 • Discovered in gamma-rays but strong X-ray source • LMXB • 15 M_sun BH • K giant companion Fender & Belloni 2004 The Transient Universe: AY 250 Spring 2007
Variability on Wide Range of Time Scales RXTE ASM The Transient Universe: AY 250 Spring 2007
Coupling Between Hardness, Temperature, and Radius The Transient Universe: AY 250 Spring 2007
Well Defined X-ray States Soft Hard Cool, distant disk Hot, close disk The Transient Universe: AY 250 Spring 2007 Markward et al 1999
Temperature Photon Index The Transient Universe: AY 250 Spring 2007
Superluminal Motion The Transient Universe: AY 250 Spring 2007
Coupled Radio/X-ray Activity The Transient Universe: AY 250 Spring 2007
Comparison to AGN • Tau ~ M^-1/2 • Jet Quenching at 1 -10% L_EDD Triangles: XRB Squares: AGN The Transient Universe: AY 250 Spring 2007
Chandra Observations of the Galactic Center • 1 Msec • 2300 sources • < 10 multi-wavelength counterparts Muno et al 2002 The Transient Universe: AY 250 Spring 2007
Foreground Separation The Transient Universe: AY 250 Spring 2007
Galactic X-ray Sources The Transient Universe: AY 250 Spring 2007
GC Transients The Transient Universe: AY 250 Spring 2007
Overabundance of Transients in Central Parsec The Transient Universe: AY 250 Spring 2007
LMXBs Dynamical friction drives compact objects to GC Three-body interactions produces LMXB HMXB Two Explanations for Transient Overdensity The Transient Universe: AY 250 Spring 2007 Ghez et al 2006
One LMXB Known X-ray eclipses Porquet et al 2005 Double-lobe radio source Bower et al 2005 The Transient Universe: AY 250 Spring 2007