MAXI/GSC detection of a possible flare from an M dwarf binary EQ Peg

Details MAXI/GSC detection of a possible flare from an M dwarf binary EQ Peg MAXI/GSC detection of a possible flare from an M dwarf binary EQ Peg

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3107....1m&link_type=abstract

The Astronomer's Telegram, #3107

Astronomy and Astrophysics

Astronomy

X-Ray, Binary, Star, Transient

Scientific paper

At a scan transit starting at 2011-01-13T06:38 (UT) (=MJD 55574.277), MAXI/GSC detected a transient X-ray source with a 4-10 keV flux of 80 +- 20 mCrab. The coordinates of the source were (R.A., Dec.) = (353.06, 19.90) = (23h 32m 13s, +19d 54' 54") (J2000) with statistical and systematic uncertainties of 0.1 and 0.2 degrees. Within the error circle is EQ Peg, an M dwarf binary at a distance of 6.25 pc.

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