A 117-day Period in IGR J19294+1816

Details A 117-day Period in IGR J19294+1816 A 117-day Period in IGR J19294+1816

Apr 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009atel.2008....1c&link_type=abstract

The Astronomer's Telegram, #2008

Astronomy and Astrophysics

Astronomy

4

X-Ray, Binaries, Neutron Stars, Pulsars, Transients

Scientific paper

An analysis of the light curve of IGR J19294+1816 (Turler et al, ATel #1997) from the Swift/BAT hard X-ray transient monitor covering 2006 January 1 through 2009 April 2 reveals a strong signal with a period of 117 days. We associate this period with the orbital period of the binary system. The power spectrum of the light curve shows strong peaks near 117 days and its harmonic near 58 days. A folding analysis also reveals a modulation near 117 days.

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