The optical counterpart to the transient X-ray pulsar SAX J2103.5+4545

Details The optical counterpart to the transient X-ray pulsar SAX J2103.5+4545 The optical counterpart to the transient X-ray pulsar SAX J2103.5+4545

Aug 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003atel..173....1r&link_type=abstract

The Astronomer's Telegram, #173

Astronomy and Astrophysics

Astronomy

13

Optical, Binaries, Pulsars, Transients

Scientific paper

We report observations of the likely optical counterpart to the 358.61-s X-ray pulsar SAX J2103.5+4545 (Hulleman et al. 1998, A&A, 337,L25). Optical photometric observations of the field around the best-fit BeppoSAX position (R.A:=21:03:33, DEC = +45:45.0) carried out on 2003 June 8.96 with the 1.3-m telescope of the Skinakas Observatory (Crete, Greece) revealed several Hα emitters but only one inside the ~2arc-min BeppoSAX radius error circle.

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