Discovery of the orbital period in the Swift/Bat data of the highly absorbed HMXB IGR J17354-3255.
Abstract
We analyzed the data collected along the 54 months of the Swift-BAT survey of the highly absorbed HMXB IGR J17354-3255 (Kuulkers, ATEL #874; Vercellone, ATEL #2019; Tomsick, ATEL #2022; Bulgarelli, ATEL #2017). The source is detected in the all-sky mosaic image obtained in the 15-50 keV energy band with a significance of 10 standard deviations. We performed a timing analysis on the BAT light curve in the same energy range using a folding search technique.
- Publication:
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The Astronomer's Telegram
- Pub Date:
- May 2010
- Bibcode:
- 2010ATel.2596....1D
- Keywords:
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- X-ray;
- Binaries;
- Neutron Stars;
- Stars