A Study of Pulse Profile Variations from EXO 2030+375 with BATSE

Details A Study of Pulse Profile Variations from EXO 2030+375 with BATSE A Study of Pulse Profile Variations from EXO 2030+375 with BATSE

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994aas...18510209p&link_type=abstract

American Astronomical Society, 185th AAS Meeting, #102.09; Bulletin of the American Astronomical Society, Vol. 26, p.1485

Astronomy and Astrophysics

Astronomy

Scientific paper

A study of pulse profile variations from the Be/x-ray transient EXO 2030+375 is presented. This transient exhibited luminosity--dependent variations in its pulse profile during initial observations by EXOSAT in 1985 (Parmar et al. 1989, ApJ, 338, 359; Parmar, White, and Stella, 1989, ApJ, 338, 373). The Large Area Detectors (LADs) of the Burst and Transient Source Experiment (BATSE) on board the Compton Gamma--Ray Observatory (CGRO) have been used to view EXO 2030+375 on sixteen occasions. The study presented here is based on these BATSE observations.

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