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ASCA Observations of White Dwarfs, Neutron Stars and Black Holes
Published online by Cambridge University Press: 25 May 2016
Extract
ASCA, the fourth Japanese X-ray astronomy satellite, was launched by the Institute of Space and Astronautical Science (ISAS) on 1993 February 20. ASCA is designed to be a high-capability X-ray observatory (Tanaka et al. 1994). It is equipped with nested thin-foil mirrors which provide a large effective area over a wide energy range from 0.5 to 10 keV. Two different types of detectors, CCD cameras (SIS) and imaging gas scintillation proportional counters (GIS) are employed as the focal plane instruments.
- Type
- 5 X-ray Binaries
- Information
- Symposium - International Astronomical Union , Volume 165: Compact Stars in Binaries , 1996 , pp. 321 - 331
- Copyright
- Copyright © Kluwer 1996