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Iron K Emission Lines in the Energy Spectra of Low‐Mass X‐Ray Binaries Observed withASCA
2000
Astrophysical Journal Supplement Series
ASCA archive data of 20 low-mass X-ray binaries (LMXBs) were analyzed to study the iron K emission lines. The LMXBs analyzed here include Z sources, atoll sources, dippers, bursters, and ADC (accretion disk corona) sources. We paid particular attention to reducing systematic errors for the estimation of line parameters, and the combination of SIS and GIS, which have di †erent energy resolutions, was found to be very useful for this purpose. We detected signiÐcant iron lines from about one-half
doi:10.1086/317374
fatcat:o3tda3tyhzd2dccxgnz5m63754