Chandra follow-up observation of the Crab nebula after the very high energy flare

Details Chandra follow-up observation of the Crab nebula after the very high energy flare Chandra follow-up observation of the Crab nebula after the very high energy flare

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2994....1f&link_type=abstract

The Astronomer's Telegram, #2994

Astronomy and Astrophysics

Astronomy

2

X-Ray, Supernova Remnant, Pulsar

Scientific paper

A Chandra TOO observation of the inner part of the Crab nebula has been performed on 2010 Oct 28 from 17:40 and 19:41 UT to monitor the evolution of the small scale structures in the region of the inner ring after the GeV flare detected by AGILE and FERMI on 2010-09-19 (ATels #2855 and #2861).
During a previous observation, performed on 2010-09-28 from 05:05 to 07:01 UT (ATel #2882), a series of three bright knots were noticed on the inner ring, at about 6 arcsec SE of the pulsar, in the region of apparent intersection with the jet.

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