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Once, years ago, listening to a recording of Mozart's Requiem Mass, Ray remarked, in that bravado way in which the young speak of dying, "Promise me you'll play that at my funeral".
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The X-ray spectra of low mass X-ray binaries (LMXB) can change on short time-scales, making it difficult to follow their spectral characteristics in detail through model fitting.
The association with blue supergiants, the spectral properties similar to those of accreting pulsars and the detection, in a few cases, of X-ray pulsations, confirm that these transients are High Mass X-ray Binaries.
We discuss millisecond period brightness oscillations and surface atomic spectral lines observed during type I X-ray bursts from a neutron star in a low mass X-ray binary system.
The burster and dipper Low Mass X-ray Binary (LMXB) 4U1915-05 (also known as XB1916-053) was observed by the Rossi X-ray Timing Explorer (RXTE) 19 times for a total exposure of 140 ks between 1996 February and October.
Attention has also been given to the problem of tuberculosis; centres have been established in every governorate, and mass X-ray and immunization campaigns have been carried out.
The area is at the confluence of three remarkable land-and-sea ecosystems; the great roiling mass of rays provided the first clue, along with the dozens of dolphins that frolicked in ever-present nonchalance just offshore.
High mass X-ray binary (HMXB) pulsars are of two types, persistent and transient.
Low mass X-ray binaries, which contain neutron stars, provide a number of methods to constrain the stellar parameters.
X-ray dipping in the black hole binary Cygnus X-1, the Galactic jet source GRO J1655-40 and in low mass X-ray binaries is discussed.
Only four of the sources have exhibited stable super-orbital periods over intervals of several years, and three of these are classed as high mass X-ray binaries.
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