IGR J11435-6109: Faded, but Variable - Possibly ~ 166 s Pulsations

Astronomy and Astrophysics – Astronomy

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X-Ray, Binaries, Pulsars, Transients

Scientific paper

On Dec. 4, 2004 at 03:42 UT RXTE observed the source IGR J11435-6109 that was recently discovered with INTEGRAL's IBIS/ISGRI. (ATEL #350). The pointing position was offset to insure no contribution in the PCA from nearby 4U 1145-619 and 1E1145.1-6141. An average net count rate of 1.7/s was observed over 896 s. Variations of about 50% were notable, which could be due to a noisy pulsation.

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