X-ray and optical-to-infrared follow-up observations of the transient X-ray burster SAX J1810.8-2609

DOI: 
Publication date: 
01/01/1999
Main author: 
Greiner J.
IAA authors: 
Castro-Tirado, A.J.
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
Publication type: 
Article
Volume: 
308
Pages: 
L17-L21
Number: 
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.
Database: 
SCOPUS
Keywords: 
Accretion, accretion discs; Infrared: stars; Stars: binaries: general; Stars: individual: SAX J1810.8-2609 (≡ RX J1810.7-2609); X-rays: stars