Authors:
Greiner J., Castro-Tirado A.J., Boller Th., Duerbeck H.W., Covino S., Israel G.L., Linden-Vørnle M.J.D., Otazu-Porter X.
Journal:
Monthly Notices of the Royal Astronomical Society
Abstract:
We have performed a ROSAT follow-up observation of the X-ray transient SAX J1810.8-2609 on 1998 March 24 and detected a bright X-ray source (named RX J1810.7-2609) which was not detected during the ROSAT all-sky survey in September 1990. Optical-to-infrared follow-up observations of the 10″ radius ROSAT HRI X-ray error box revealed one variable object (R = 19.5 ± 0.5 on March 13, R > 21.5 on 1998 August 27) which we tentatively propose as the optical/IR counterpart of RX J1810.7-2609 ≡ SAX J1810.8-2609.
Keywords:
Accretion, accretion discs; Infrared: stars; Stars: binaries: general; Stars: individual: SAX J1810.8-2609 (≡ RX J1810.7-2609); X-rays: stars