Properties of a B0 I stellar wind and interstellar grains derived from GINGA observations of the binary X-ray pulsar 4U 1538-52

Astrophysical Journal February 1994. 1994ApJ...422..336C.

ECLIPSING BINARY STARS, GINGA SATELLITE, INTERSTELLAR EXTINCTION, INTERSTELLAR MATTER, MONTE CARLO METHOD, PROPORTIONAL COUNTERS, Pulsars, PULSE AMPLITUDE, RADIATION ABSORPTION, STELLAR WINDS, X RAY ASTRONOMY, X RAY STARS, X-ray spectra