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- W88336461 abstract "We discuss the optical identification of 9 Be/X-ray binary optical counterparts of X-ray sources in the Magellanic clouds, most of them discovered in ROSAT observations. Imaging CCD photometry (using BV R C and Hα filters) was employed to search the typically 20 arcsec radius error circles for early-type stars exhibiting Hα emission. Spectroscopy of 5 candidates confirmed the presence of Hα emission. Based on the positional coincidences, we propose Be star optical counterparts to all of 9 X-ray sources: 6 from ROSAT and one each from ASCA, EXOSAT and HEAO-1. All of the sources exhibit the typical X-ray characteristics of Be/neutron star X-ray binaries: transient nature or strong variability, relatively hard X-ray spectra and, in 5 cases, detections of probable neutron star spin periods in the range 8.9 to 91.1 seconds." @default.
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- W88336461 date "1999-01-01" @default.
- W88336461 modified "2023-09-25" @default.
- W88336461 title "Optical Counterparts to Be/X-ray Binaries in the Magellanic Clouds" @default.
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- W88336461 doi "https://doi.org/10.1017/s0074180900204002" @default.
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