A variable star in the vicinity of the soft gamma-ray repeater 1806 - 20

Details A variable star in the vicinity of the soft gamma-ray repeater 1806 - 20 A variable star in the vicinity of the soft gamma-ray repeater 1806 - 20

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993mnras.263l...1i&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 263, no. 1, p. L1-L5.

Astronomy and Astrophysics

Astronomy

1

Gamma Ray Astronomy, Gamma Ray Bursts, Star Distribution, Variable Stars, Astronomical Photography, Sky Surveys (Astronomy), Stellar Color, Stellar Spectra

Scientific paper

The APM facility in Cambridge has been used to search archive UK Schmidt
Telescope photographic plates for an optical counterpart of SGR 1806 -
20. The search has revealed a late-type variable star just outside the
revised 3 sigma error box. A low-resolution spectrum of the star
suggests that it is almost undoubtedly an M9 Mira.

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