Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296..483k&link_type=abstract
In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 1: X Ray Binaries p 483-484 (SEE N90-25711 19-89)
Astronomy and Astrophysics
Astronomy
Ginga Satellite, Pulsars, Pulse Amplitude, Satellite Observation, Stellar Models, X Ray Spectra, Energy Bands, Japanese Space Program, Pulse Duration, Stellar Parallax, Stellar Spectra, X Ray Sources
Scientific paper
The discovery of six X ray pulsars and several candidates of X ray pulsars is reported. These new pulsars and candidates show a high concentration towards the Scutum region. The pulse profiles, in several energy bands and X ray spectra of these new X ray pulsars are presented. The best fit models are given. The model used is a power law plus exponential cut (if necessary). The positions and best fit parameters of the X ray pulsars are shown.
Koyama Katsuji
Takeuchi Yoshitaka
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