Discovery of the optical counterpart to the ASCA transient AX 1845.0-0433

Details Discovery of the optical counterpart to the ASCA transient AX 1845.0-0433 Discovery of the optical counterpart to the ASCA transient AX 1845.0-0433

Jul 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996mnras.281..333c&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 281, Issue 1, pp. 333-338.

Astronomy and Astrophysics

Astronomy

15

Binaries: General, Stars: Emission-Line, Be, Pulsars: General, Infrared: Stars, X-Rays: Stars

Scientific paper

We report observations which identify the optical/IR counterpart to the
X-ray transient AX 1845.0-0433. The counterpart is suggested to be an
O9.5 supergiant star with weak Balmer emission lines. Its distance is
estimated to be 3.6 kpc - consistent with the distance derived from
X-ray measurements.

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