** This Symbiotic Fascination by Charlee Jacob

** ( Medicine, Lungs ; Tuberculosis: Treatment ; X-ray )

** ( Medicine, Lungs ; Tuberculosis: Treatment ; X-ray: Research )

** ( Medicine, Lungs ; Tuberculosis: Treatment ; X-ray: Research. India )

** ( Medicine, Lungs ; Tuberculosis: Treatment ; X-ray: Research. India ' 1950 )

** X-ray

** Screen films ( conventional X-ray films ).

** Nondestructive testing ( NDT ) film ( as the exclusive manufacturer of General Electric's NDT X-ray films and related chemistry.

** Acquisition of CEA AB ( X-ray film products ).

** Acquisition of Sterling Diagnostic Imaging ( X-ray film and equipment ).

** Acquisition of the German company Seifert and the American company Pantak, producers of industrial X-ray equipment for non-destructive testing applications.

** Soft X-ray transients ( SXTs )

** Super soft X-ray sources or Super soft sources ( SSSs ),( SSXB )

** Be / X-ray binaries ( BeXRBs )

** Supergiant X-ray binaries ( SGXBs )

** Supergiant Fast X-ray Transients ( SFXTs )

** X-ray bursters

** X-ray pulsars

** Microquasars ( radio-jet X-ray binaries that can house either a neutron star or a black hole )

** chest X-ray, CT scan and 3D reconstruction images or CT virtual bronchoscopy, bronchial angiography.

** X-ray computed tomography ( CT )

** Visible / UV / X-ray spectrometers – temperatures and densities

** Soft X-ray cameras to examine MHD properties of plasmas

** Hard X-ray monitors

** X-ray and gamma radiation are best absorbed by atoms with heavy nuclei ; the heavier the nucleus, the better the absorption.

** Vorbis binaries at Rarewares

** Eclipsing binaries, double stars where, as seen from Earth's vantage point the stars occasionally eclipse one another as they orbit.

** Eclipsing binaries — In the last decade, measurement of eclipsing binaries ' fundamental parameters has become possible with 8 meter class telescopes.

** FreeBSD's Linux Compatibility Layer, which enables binaries built specifically for Linux to run on FreeBSD with the same way as the native FreeBSD API layer.

** Planets: Phoebe, the Aeolus asteroid belt, the gas giant Hestia ( 17 moons, including binaries Rhea and Kronos ) with Canceron & Aerilon at Hestia's L4 and L5, Aquaria, and Styx.

** Compiled binaries:

The observations show that the cloud is asymmetrical and matches the pattern of X-ray binaries ( binary star systems containing black holes or neutron stars ), mostly on one side of the galactic center.

Of the first five luminous LMC X-ray binaries: LMC X-1, X-2, X-3, X-4, and A 0538-66 ( detected by Ariel 5 at A 0538-66 ); LMC X-2 is the only one that is a bright low-mass X-ray binary system ( LMXB ) in the LMC.

Several types of astrophysical objects emit, fluoresce, or reflect X-rays, from galaxy clusters, through black holes in active galactic nuclei ( AGN ) to galactic objects such as supernova remnants, stars, and binary stars containing a white dwarf ( cataclysmic variable stars and super soft X-ray sources ), neutron star or black hole ( X-ray binaries ).

X-1 is the prototype for the massive X-ray binaries although it falls on the borderline, ~ 2 M < sub >☉</ sub >, between high-and low-mass X-ray binaries.

High-mass X-ray binaries ( HMXBs ) are composed of OB supergiant companion stars and compact objects, usually neutron stars ( NS ) or black holes ( BH ).

Supergiant X-ray binaries ( SGXBs ) are HMXBs in which the compact objects orbit massive companions with orbital periods of a few days ( 3 – 15 d ), and in circular ( or slightly eccentric ) orbits.

Observations are revealing a growing number of recurrent X-ray transients, characterized by short outbursts with very fast rise times ( tens of minutes ) and typical durations of a few hours that are associated with OB supergiants and hence define a new class of massive X-ray binaries: Supergiant Fast X-ray Transients ( SFXTs ).

In X-ray binaries, the compact object can be either a neutron star or a black hole.

High-mass X-ray binaries contain a young, early type, high-mass donor star which transfers mass by its stellar wind, while low-mass X-ray binaries are semidetached binaries in which gas from a late-type donor star overflows the Roche lobe and falls towards the neutron star or black hole.

The similarities between the emissions of X-ray binaries such as HDE 226868 / Cygnus X-1 and active galactic nuclei suggests a common mechanism of energy generation involving a black hole, an orbiting accretion disk and associated jets.

The Small Magellanic Cloud contains a large and active population of X-ray binaries.

Recent star formation has led to a large population of massive stars and high-mass X-ray binaries ( HMXBs ) which are the relics of the short-lived upper end of the initial mass function.

The young stellar population and the majority of the known X-ray binaries are concentrated in the SMC ’ s Bar.