Swift detection of a superflare from CC Eridani

Details Swift detection of a superflare from CC Eridani Swift detection of a superflare from CC Eridani

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1787....1e&link_type=abstract

The Astronomer's Telegram, #1787

Astronomy and Astrophysics

Astronomy

X-Ray, Gamma Ray, Variables, Stars

Scientific paper

At 11:22:52 UT on 2008 October 16, the Swift BAT triggered on a superflare from the the binary system CC Eridani. This system consists of a dK7 and dM3 star, with an orbital period of 1.57 days, and is at a distance of 11.5 pc. Swift slewed to the system immediately, and the XRT began observing the source 147.2 s after the trigger. The BAT light curve shows a rise in intensity beginning near T-200s reaching a plateau around T=0 s.

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