MAXI/GSC detection of a possible activity from Swift J1922.7-1716

Details MAXI/GSC detection of a possible activity from Swift J1922.7-1716 MAXI/GSC detection of a possible activity from Swift J1922.7-1716

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3548....1n&link_type=abstract

The Astronomer's Telegram, #3548

Astronomy and Astrophysics

Astronomy

X-Ray, Binary

Scientific paper

MAXI/GSC has detected an enhanced X-ray emission from a position consistent with Swift J1922.7-1716. The observed X-ray flux averaged over 8 days from 2011-08-01 to 2011-08-08 (UT) was 10.2 ± 2.7 mCrab in the 2-20 keV band. The best-fit source position is (R.A., Dec)=(290.75, -17.35)=(19 23 00.00,-17 21 00.0) (J2000), which includes a systematic uncertainty of 0.2 degree (90% containment radius).

Affiliated with

Also associated with

No associations

Rating

MAXI/GSC detection of a possible activity from Swift J1922.7-1716 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with MAXI/GSC detection of a possible activity from Swift J1922.7-1716, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and MAXI/GSC detection of a possible activity from Swift J1922.7-1716 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1021988