Optical monitoring of IGR J00291+5934

Details Optical monitoring of IGR J00291+5934 Optical monitoring of IGR J00291+5934

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005atel..395....1b&link_type=abstract

The Astronomer's Telegram, #395

Astronomy and Astrophysics

Astronomy

7

Optical, Binaries, Neutron Stars, Pulsars

Scientific paper

We have photometrically monitored the optical transient associated with the accretion-powered millisecond pulsar IGRJ00291+5934 (ATEL352,353,354,363) during the period of December 11, 2004 - January 13, 2005, with Russian-Turkish 1.5-m optical telescope (RTT150) at Bakirlitepe (Antalya, Turkey). The R-band light curve is shown at http://db.rsdc.rssi.ru/IGRJ00291+5934/fig1.jpg Optical flux decay is nearly exponential with e-folding time 5.66+/-0.2 days.

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