Discovery of the orbital period in the Swift/Bat data of the highly absorbed HMXB IGR J17354-3255.

Details Discovery of the orbital period in the Swift/Bat data of the highly absorbed HMXB IGR J17354-3255. Discovery of the orbital period in the Swift/Bat data of the highly absorbed HMXB IGR J17354-3255.

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2596....1d&link_type=abstract

The Astronomer's Telegram, #2596

Astronomy and Astrophysics

Astronomy

1

X-Ray, Binaries, Neutron Stars, Stars

Scientific paper

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.

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